This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0436 Cen,2461120.7139,12.48,0.05,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
V0436 Cen 20260321.2139 12.48CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:59.87 -37:40:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20_00sec_-14_90C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.2139 2461120.7139 10.96 11:09:16.77 -33:37:10.8
279.67533 24.59719 galactic Hya Second-epoch detections are separated by 0.3" and 5.0 pix
The object was found in VSX 0" BH Hya
Type: M
# Max. Min./Amp. JD0 Period
11.500 pg 15.500 pg 2427850.00000 211.000000000000 Me
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BH Hya,2461120.7139,10.96,0.05,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
BH Hya 20260321.2139 10.96CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:09:16.77 -33:37:10.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20_00sec_-14_90C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.2139 2461120.7139 9.23 11:41:16.61 -33:42:33.6
286.60063 26.92763 galactic Hya Second-epoch detections are separated by 0.2" and 4.6 pix
The object was found in VSX 1" DN Hya
Type: M
# Max. Min./Amp. JD0 Period
11.400 pg 14.400 pg 2428190.00000 182.400000000000 Me
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DN Hya,2461120.7139,9.23,0.05,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
DN Hya 20260321.2139 9.23CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:41:16.61 -33:42:33.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20_00sec_-15_00C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20_00sec_-14_90C_LIGHT_0201_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20_00sec_-15_00C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.88132895 21.01.2026 09:08:56.821 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
First image: 2461061.88132895 21.01.2026 09:08:56.821 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
Last image: 2461120.71413675 21.03.2026 05:08:11.415 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.44
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): 5354
Objects passed selection criteria: 5351
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 5170.5
Average stars matched: 5065.75 (97.9741 %)
Memory usage VmPeak: 111872 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 21 00:34:12 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: 2461061.88132895 21.01.2026 09:08:56.821 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
First image: 2461061.88132895 21.01.2026 09:08:56.821 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
Last image: 2461120.71413675 21.03.2026 05:08:11.415 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.15
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: 14 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): 36241
Objects passed selection criteria: 36210
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 34436.5
Average stars matched: 33362.5 (96.8812 %)
Memory usage VmPeak: 139436 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 21 00:35:11 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-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
SExtractor catalog cache: saved Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat to cache
SExtractor catalog cache: saved Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.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: 2461120.71359498
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'
Plate-solving the images
wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits exists and is non-empty
Saving wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits to local_wcs_cache/
'wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits' -> 'local_wcs_cache/wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits'
wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits exists and is non-empty
Saving wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits to local_wcs_cache/
'wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits' -> 'local_wcs_cache/wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits'
wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits exists and is non-empty
Saving wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits to local_wcs_cache/
'wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits' -> 'local_wcs_cache/wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits'
wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
Saving wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits to local_wcs_cache/
'wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:28:36.527 -34:00:12.37
Second-epoch image center 11:28:42.436 -34:00:15.46
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:28:36.527 -34:00:12.37
Second-epoch image center 11:28:43.133 -33:59:48.42
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:28:42.436 -34:00:15.46
Second-epoch second image center 11:28:43.133 -33:59:48.42
Angular distance between the image centers 0.00789 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits &> /tmp/tmp.QGnGTyQXM2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits &> /tmp/tmp.fzGvh0z6Xb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits &> /tmp/tmp.taqsKiyAWZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.tFdcGGpAbH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits and wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits and wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
Found non-empty wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits and wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
The reference image (wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits) and catalog (wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat) found
'wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5394 out of 6358 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.695113
a=0.000000 b=1.000000 c=22.695113
From vast_summary.log: estimated ref. image limiting mag.: -8.44
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.26
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
2.3 pix Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
2.7 pix fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
2.7 pix fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Limiting magnitude estimates:
14.3 mag. Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
14.2 mag. Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
14.0 mag. fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
14.0 mag. fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.3 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QGnGTyQXM2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits' -> 'wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
WCS-calibrated image found: wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
Checking if the catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat corresponding to the image wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat corresponding to the image wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
WCS catalog name: wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=6358
Got 6358 stars (including 5923 good ones) from the SExtractor catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
util/solve_plate_with_UCAC5 got 6358 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits -region wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.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.fzGvh0z6Xb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits' -> 'wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
WCS_IMAGE_NAME=wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
WCS-calibrated image found: wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
Checking if the catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat corresponding to the image wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits alredy exist and is non-empty...
Catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat corresponding to the image wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
WCS catalog name: wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=6398
Got 6398 stars (including 5955 good ones) from the SExtractor catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat
util/solve_plate_with_UCAC5 got 6398 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits -region wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.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.taqsKiyAWZ (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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
WCS-calibrated image found: wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
Checking if the catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
WCS catalog name: wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=320, passed=5813
Got 5813 stars (including 5488 good ones) from the SExtractor catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 5813 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits -region wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.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.tFdcGGpAbH (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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=310, passed=5788
Got 5788 stars (including 5475 good ones) from the SExtractor catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 5788 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits'
Saving fully-calibrated image wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits'
Saving fully-calibrated image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits'
Saving fully-calibrated image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits'
Preparing the HTML report for the field Hya-15-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20340.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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
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Considering the candidate 20301_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 20301_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:41:16.62 -33:42:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.22, MAG_FAINT_SEARCH_LIMIT=10.20)GAIADR2_OUTPUT=# 0.533 3477417870319764864 175.31937373111 -33.70922688457 8.6340 7.5971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20322_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 20322_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:10:09.22 -35:59:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 1.161 5400500300424222464 167.53805534990 -35.98589178058 11.6377 9.8921 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20325_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 20325_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:09:16.77 -33:37:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 0.415 5403227879534467072 167.31987126467 -33.61960705235 10.8580 9.6406 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20335_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 20335_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:30:34.27 -36:26:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 1.070 5398212044927910784 172.64300816760 -36.44023146061 9.9955 8.6389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20340_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 20340_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:42:27.67 -35:38:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 0.233 3464726276322657792 175.61537044772 -35.63768433990 11.2040 10.7068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Hya-15-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-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
SExtractor catalog cache: saved Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat to cache
SExtractor catalog cache: saved Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
Creating symlink local_wcs_cache/wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits exists and is non-empty
wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits exists and is non-empty
wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits exists and is non-empty
wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:28:36.527 -34:00:12.37
Second-epoch image center 11:28:42.436 -34:00:15.46
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:28:36.527 -34:00:12.37
Second-epoch image center 11:28:43.133 -33:59:48.42
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:28:42.436 -34:00:15.46
Second-epoch second image center 11:28:43.133 -33:59:48.42
Angular distance between the image centers 0.00789 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits &> /tmp/tmp.XHZbZiir0d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits &> /tmp/tmp.ThcAdcblLH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits &> /tmp/tmp.iSvavDX8eF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.iHhvy3KILN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits and wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits and wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
Found non-empty wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits and wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
The reference image (wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits) and catalog (wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat) found
'wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 8006 out of 42373 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.517126
a=0.000000 b=1.000000 c=22.517126
From vast_summary.log: estimated ref. image limiting mag.: -8.15
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 20 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
2.3 pix Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
2.5 pix fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
2.5 pix fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Limiting magnitude estimates:
14.4 mag. Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
14.3 mag. Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
14.2 mag. fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
14.2 mag. fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.5 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.XHZbZiir0d (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits' -> 'wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
WCS-calibrated image found: wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
Checking if the catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat corresponding to the image wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat corresponding to the image wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
WCS catalog name: wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1622, passed=42371
Got 42371 stars (including 40679 good ones) from the SExtractor catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat
util/solve_plate_with_UCAC5 got 42371 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits -region wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.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.ThcAdcblLH (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits' -> 'wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
WCS_IMAGE_NAME=wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
WCS-calibrated image found: wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
Checking if the catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat corresponding to the image wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits alredy exist and is non-empty...
Catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat corresponding to the image wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
WCS catalog name: wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1555, passed=41899
Got 41899 stars (including 40273 good ones) from the SExtractor catalog wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat
util/solve_plate_with_UCAC5 got 41899 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits -region wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.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.iSvavDX8eF (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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
WCS-calibrated image found: wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
Checking if the catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
WCS catalog name: wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1310, passed=34401
Got 34401 stars (including 33053 good ones) from the SExtractor catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 34401 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits -region wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.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.iHhvy3KILN (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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1283, passed=34405
Got 34405 stars (including 33088 good ones) from the SExtractor catalog wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 34405 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/wcs_Hya-15-Q2b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits
Saving fully-calibrated image wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/wcs_Hya-15-Q2b1x1_2026-01-21_03-09-51_20.00sec_-14.90C_LIGHT_0436.fits
Saving fully-calibrated image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-07-24_20.00sec_-14.90C_LIGHT_0201.fits
Saving fully-calibrated image wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.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_2026-03-21_CI_Hya-15-Q2b1x1_003029_TTUQ2b1x1_8348_VXrYwJQ1/wcs_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202.fits
Preparing the HTML report for the field Hya-15-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52964.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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: 3s
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Considering the candidate 52813_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52813_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:36:06.39 -30:46:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.286 3478968594034958464 174.02736149371 -30.77205678471 13.7396 13.0413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52814_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52814_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:38:51.85 -30:02:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.547 3480517015644343808 174.71594286314 -30.03379093328 13.5871 13.0523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52818_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52818_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:40:29.72 -30:22:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.178 3480452384976656640 175.12452940177 -30.37814939989 13.5484 12.7539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52822_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52822_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:56:57.27 -32:54:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.460 5450242343903578368 164.23852218319 -32.91107233411 13.6522 13.0545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52825_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52825_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:43:19.41 -32:06:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.010 3477822387521727232 175.83086099199 -32.11186375873 13.3270 12.8414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52830_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52830_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:50:11.09 -31:23:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.472 3479250584406285568 177.54517837464 -31.39634080788 13.3807 12.8710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52857_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52857_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:10:09.21 -35:59:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 0.975 5400500300424222464 167.53805534990 -35.98589178058 11.6377 9.8921 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52951_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52951_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:59:07.99 -34:20:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.905 5401863179445996160 164.78343724059 -34.34919599668 12.5223 12.0902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52964_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
Preparing report for the candidate 52964_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
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Considering the candidate 52970_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 52970_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:32:50.17 -31:50:11.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 53040_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 53040_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:57:11.28 -35:10:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.520 3464105808166136704 179.29592846582 -35.17782252671 12.8210 12.1768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53059_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 53059_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 10:59:08.78 -35:57:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.485 5401063520958249472 164.78607880721 -35.95519649910 12.0771 10.3526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53123_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 53123_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:45:20.48 -32:30:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.890 3477606780162878976 176.33471457334 -32.50744159069 13.5098 12.9077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53145_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 53145_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:28:10.77 -31:13:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.429 3481522862624583936 172.04543308537 -31.22252306182 13.7926 13.2889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53152_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 53152_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:44:44.43 -29:40:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.563 3480426099775309056 176.18472360646 -29.66924141043 13.7665 13.1511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53228_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 53228_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:44:20.42 -30:00:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.385 3480388166624176640 176.08471237940 -30.01251710163 13.8954 13.4814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53267_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 53267_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks
**** FOUND 11:17:00.46 -35:33:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.333 5399059218636778368 169.25194350637 -35.56288245243 13.7436 13.1741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53284_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202
The candidate 53284_fd_Hya-15-Q2b1x1_2026-03-21_00-08-11_20.00sec_-15.00C_LIGHT_0202 did not pass the final checks