This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 20.2759 2461119.7759 14.02 13:35:40.93 -24:04:20.0
315.72235 37.69820 galactic Hya Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:35:40.93 -24:04:20.0 (user input) | T | P | (position from user input) J-Ks=2.557+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
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
target,2461119.7759,14.02,0.05,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
target 20260320.2759 14.02CV 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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:35:40.93 -24:04:20.0 ;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-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20_00sec_-15_00C_LIGHT_0285_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20_00sec_-15_00C_LIGHT_0284_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20_00sec_-15_00C_LIGHT_0285_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
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
VARIABLE_NAME,2461119.7759,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.2759 12.84CV 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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:42:40.09 -23:17:31.3 ;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-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20_00sec_-15_00C_LIGHT_0285_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20_00sec_-15_00C_LIGHT_0284_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20_00sec_-15_00C_LIGHT_0285_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
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
VARIABLE_NAME,2461119.7759,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.2759 13.66CV 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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:32:34.13 -23:14:38.2 ;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-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20_00sec_-15_00C_LIGHT_0285_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20_00sec_-15_00C_LIGHT_0284_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20_00sec_-15_00C_LIGHT_0285_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20_00sec_-15_00C_LIGHT_0284_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: 2461058.93459012 18.01.2026 10:25:38.586 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
First image: 2461058.93459012 18.01.2026 10:25:38.586 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
Last image: 2461119.77613968 20.03.2026 06:37:28.468 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.23
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: 2 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): 4745
Objects passed selection criteria: 4741
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: 4551.75
Average stars matched: 4375.75 (96.1334 %)
Memory usage VmPeak: 111352 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 02:46:04 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: 2461058.93459012 18.01.2026 10:25:38.586 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
First image: 2461058.93459012 18.01.2026 10:25:38.586 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
Last image: 2461119.77613968 20.03.2026 06:37:28.468 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 70
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.91
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: 10 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): 32797
Objects passed selection criteria: 32736
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 31353
Average stars matched: 30170.8 (96.2292 %)
Memory usage VmPeak: 135860 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 02:46:48 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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
SExtractor catalog cache: saved Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat to cache
SExtractor catalog cache: saved Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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: 2461119.77557887
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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits exists and is non-empty
Saving wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits to local_wcs_cache/
'wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits' -> 'local_wcs_cache/wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits'
wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits exists and is non-empty
Saving wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits to local_wcs_cache/
'wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits' -> 'local_wcs_cache/wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits'
wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits exists and is non-empty
Saving wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits to local_wcs_cache/
'wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits' -> 'local_wcs_cache/wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits'
wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits exists and is non-empty
Saving wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits to local_wcs_cache/
'wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits' -> 'local_wcs_cache/wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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 13:26:23.700 -25:59:53.07
Second-epoch image center 13:26:46.595 -26:03:02.13
Angular distance between the image centers 0.10 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 13:26:23.700 -25:59:53.07
Second-epoch image center 13:26:47.702 -26:03:44.54
Angular distance between the image centers 0.11 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 13:26:46.595 -26:03:02.13
Second-epoch second image center 13:26:47.702 -26:03:44.54
Angular distance between the image centers 0.01249 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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits &> /tmp/tmp.9jNE8Pryte
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits &> /tmp/tmp.zBooqQTLN8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits &> /tmp/tmp.TYXBL588Kk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits &> /tmp/tmp.xBH5YJFjaD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits and wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits and wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat
Found non-empty wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits and wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat
The reference image (wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits) and catalog (wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat) found
'wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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 4421 out of 5375 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.696539
a=0.000000 b=1.000000 c=22.696539
From vast_summary.log: estimated ref. image limiting mag.: -8.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
2.1 pix Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
2.6 pix fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
2.6 pix fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
Limiting magnitude estimates:
14.5 mag. Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
14.5 mag. Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
14.4 mag. fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
14.4 mag. fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (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.9jNE8Pryte (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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits' -> 'wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
WCS_IMAGE_NAME=wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
WCS-calibrated image found: wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
Checking if the catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits alredy exist and is non-empty...
Catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
WCS catalog name: wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=372, passed=5375
Got 5375 stars (including 4992 good ones) from the SExtractor catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat
util/solve_plate_with_UCAC5 got 5375 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 960 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits -region wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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.zBooqQTLN8 (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-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits' -> 'wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
WCS_IMAGE_NAME=wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
WCS-calibrated image found: wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
Checking if the catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits alredy exist and is non-empty...
Catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
WCS catalog name: wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=384, passed=5380
Got 5380 stars (including 4991 good ones) from the SExtractor catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat
util/solve_plate_with_UCAC5 got 5380 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 957 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits -region wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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.TYXBL588Kk (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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
WCS_IMAGE_NAME=wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
WCS-calibrated image found: wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
Checking if the catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
WCS catalog name: wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=313, passed=5763
Got 5763 stars (including 5445 good ones) from the SExtractor catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat
util/solve_plate_with_UCAC5 got 5763 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits -region wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.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.xBH5YJFjaD (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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
WCS_IMAGE_NAME=wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
WCS-calibrated image found: wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
Checking if the catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
WCS catalog name: wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=326, passed=5762
Got 5762 stars (including 5428 good ones) from the SExtractor catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat
util/solve_plate_with_UCAC5 got 5762 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits -region wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits'
Saving fully-calibrated image wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits'
Saving fully-calibrated image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits'
Saving fully-calibrated image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits'
Preparing the HTML report for the field Hya-13-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20282.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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20251_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 20251_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:03:20.42 -29:06:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20263_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 20263_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:28:27.08 -27:23:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20269_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 20269_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:35:25.78 -22:23:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20275_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 20275_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:23:15.52 -25:55:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20281_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 20281_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:26:28.90 -24:43:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 0.117 6193232756526343680 201.62045213384 -24.73330906782 11.4852 11.0177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20282_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 20282_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:31:33.14 -26:19:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 0.530 6189704728654650752 202.88792241948 -26.32477931304 11.6373 11.2861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.530#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-13-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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
SExtractor catalog cache: saved Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat to cache
SExtractor catalog cache: saved Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
Creating symlink local_wcs_cache/wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits exists and is non-empty
wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits exists and is non-empty
wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits exists and is non-empty
wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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 13:26:23.700 -25:59:53.07
Second-epoch image center 13:26:46.595 -26:03:02.13
Angular distance between the image centers 0.10 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 13:26:23.700 -25:59:53.07
Second-epoch image center 13:26:47.702 -26:03:44.54
Angular distance between the image centers 0.11 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 13:26:46.595 -26:03:02.13
Second-epoch second image center 13:26:47.702 -26:03:44.54
Angular distance between the image centers 0.01249 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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits &> /tmp/tmp.5EEXNNqL7z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits &> /tmp/tmp.SfCDtdUAIr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits &> /tmp/tmp.Iw4oEGiD2r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits &> /tmp/tmp.4gm751ZEsg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits and wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits and wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat
Found non-empty wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits and wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat
The reference image (wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits) and catalog (wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat) found
'wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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 5747 out of 38006 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.520085
a=0.000000 b=1.000000 c=22.520085
From vast_summary.log: estimated ref. image limiting mag.: -7.91
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.61
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
2.0 pix Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
2.5 pix fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
2.5 pix fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
Limiting magnitude estimates:
14.6 mag. Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
14.6 mag. Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
14.5 mag. fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
14.5 mag. fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5EEXNNqL7z (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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits' -> 'wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
WCS_IMAGE_NAME=wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
WCS-calibrated image found: wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
Checking if the catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits alredy exist and is non-empty...
Catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
WCS catalog name: wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1303, passed=38003
Got 38003 stars (including 36646 good ones) from the SExtractor catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat
util/solve_plate_with_UCAC5 got 38003 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 960 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits -region wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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.SfCDtdUAIr (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-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits' -> 'wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
WCS_IMAGE_NAME=wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
WCS-calibrated image found: wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
Checking if the catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits alredy exist and is non-empty...
Catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat corresponding to the image wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
WCS catalog name: wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1314, passed=37987
Got 37987 stars (including 36611 good ones) from the SExtractor catalog wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat
util/solve_plate_with_UCAC5 got 37987 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 958 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits -region wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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.Iw4oEGiD2r (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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
WCS_IMAGE_NAME=wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
WCS-calibrated image found: wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
Checking if the catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
WCS catalog name: wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1299, passed=34081
Got 34081 stars (including 32735 good ones) from the SExtractor catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat
util/solve_plate_with_UCAC5 got 34081 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits -region wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.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.4gm751ZEsg (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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
WCS_IMAGE_NAME=wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
WCS-calibrated image found: wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
Checking if the catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat corresponding to the image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
WCS catalog name: wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1351, passed=33731
Got 33731 stars (including 32339 good ones) from the SExtractor catalog wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat
util/solve_plate_with_UCAC5 got 33731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits -region wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits
Saving fully-calibrated image wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/wcs_Hya-13-Q2b1x1_2026-01-18_04-26-33_20.00sec_-14.90C_LIGHT_0502.fits
Saving fully-calibrated image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-36-40_20.00sec_-15.00C_LIGHT_0284.fits
Saving fully-calibrated image wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.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_2026-03-20_CI_Hya-13-Q2b1x1_024348_TTUQ2b1x1_9867_bSC2sFWq/wcs_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285.fits
Preparing the HTML report for the field Hya-13-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52988.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 52690_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
Preparing report for the candidate 52690_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
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Considering the candidate 52691_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 52691_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:46:03.01 -22:39:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 0.846 6288235543328240128 206.51236750773 -22.65692144608 14.2375 13.6418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52693_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 52693_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:15:36.97 -27:52:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52718_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 52718_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:28:27.06 -27:23:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52811_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
Preparing report for the candidate 52811_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
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Considering the candidate 52832_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 52832_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:52:47.01 -25:23:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52906_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 52906_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:47:44.19 -22:03:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52936_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 52936_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:39:49.03 -25:25:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.286 6190696939115266816 204.95391038425 -25.42193322815 13.6574 13.0978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52964_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 52964_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:16:20.21 -28:17:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52973_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 52973_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:52:13.23 -27:35:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52988_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
Preparing report for the candidate 52988_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
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Considering the candidate 53001_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53001_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:48:39.64 -24:11:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53010_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53010_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:50:40.70 -26:44:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53015_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53015_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:53:06.27 -24:08:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53018_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53018_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:42:59.79 -22:48:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53027_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53027_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:48:05.81 -24:06:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53044_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53044_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:44:35.85 -26:48:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.646 6178228958293133568 206.14907044892 -26.80206207958 14.0706 13.5769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53045_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53045_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:43:27.28 -27:35:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.551 6178115536796850176 205.86319474358 -27.59636859817 14.1514 13.6487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53054_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53054_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:46:00.64 -29:10:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53073_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53073_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:49:05.10 -27:18:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53082_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53082_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:52:46.95 -23:17:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.768 6287260104715551104 208.19574041468 -23.29285172399 14.3023 13.7533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53085_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53085_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:27:50.44 -25:36:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53091_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53091_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:30:01.60 -23:21:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.094 6194841685635258240 202.50688066441 -23.36092633396 14.0375 13.6043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53099_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53099_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:43:15.52 -22:41:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 0.602 6192357717069414400 205.81467930029 -22.68769442441 14.1861 13.6036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53102_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53102_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:24:39.93 -29:23:19.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)
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Considering the candidate 53103_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53103_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:35:46.31 -22:24:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53107_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53107_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:44:16.40 -23:06:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.680 6192139979407383424 206.06753394239 -23.10508961992 14.3888 13.8751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53108_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53108_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:53:02.22 -25:22:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.945 6178851934709005056 208.25953565501 -25.37499159528 13.8063 12.9747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53117_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53117_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:45:19.31 -24:59:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.077 6191053661918965760 206.33019178424 -24.98651786448 14.0768 13.5641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53119_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53119_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:47:00.78 -23:54:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.001 6191289026126856832 206.75335941024 -23.91537050465 14.2951 13.7681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53120_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53120_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:50:45.89 -26:37:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.201 6178466418444662912 207.69152917551 -26.61680184125 13.9471 13.4577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53124_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53124_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:41:57.10 -29:18:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.223 6176183316909694720 205.48771519188 -29.30095925278 13.9593 13.3779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53127_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53127_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:51:06.96 -22:07:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.794 6288334018338433664 207.77913042663 -22.11737772544 14.1394 13.5450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53128_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53128_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:47:27.12 -22:30:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.097 6288259492065902464 206.86276178426 -22.51170582371 14.0788 13.4306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53129_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53129_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 53131_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53131_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:30:57.67 -29:56:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.509 6175934655482837888 202.73982459640 -29.94708143597 13.7326 12.7911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53146_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53146_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:46:28.38 -23:54:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.120 6191266348699535872 206.61859002883 -23.91487700350 14.0179 13.4610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53147_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53147_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:45:58.14 -23:25:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 1.322 6192072359442375168 206.49199324982 -23.43232926824 14.1599 13.6150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53151_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53151_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:48:10.26 -25:03:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.344 6190829945662661120 207.04265299941 -25.05501790639 14.0979 13.5087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53152_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53152_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:50:28.43 -22:50:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.453 6287523437750427648 207.61802050313 -22.84023470216 14.1929 13.5784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53162_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53162_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:28:49.44 -29:52:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.983 6181958226856566144 202.20537944216 -29.88152145486 14.1766 13.6616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53163_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53163_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:45:36.29 -24:44:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.376 6191084070287469824 206.40081318092 -24.74377060403 14.1425 13.5966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53194_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53194_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:17:23.35 -28:54:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.060 6183196448747916032 199.34699349553 -28.91103024851 14.2188 13.5411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53197_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53197_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:29:36.18 -23:13:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.197 6195034065810413952 202.40109613307 -23.22781868094 13.9404 13.3032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53203_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53203_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:39:50.03 -24:00:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 0.375 6191965565080298112 204.95834989086 -24.00318994882 13.8222 12.9280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53211_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53211_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:21:41.14 -29:08:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.551 6183023687983387264 200.42156421176 -29.13913837647 14.1208 13.6091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53222_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53222_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:37:40.12 -22:11:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 1.442 6195478268507688704 204.41700523681 -22.18606602380 14.1070 13.5500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53252_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 53252_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:01:33.64 -29:00:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 0.653 6184553005578303488 195.39036820929 -29.01384635750 14.0396 13.4980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 30020_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 30020_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:35:25.75 -22:23:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20193_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 20193_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks
**** FOUND 13:23:15.52 -25:55:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07085_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285
The candidate 07085_fd_Hya-13-Q2b1x1_2026-03-20_01-37-28_20.00sec_-15.00C_LIGHT_0285 did not pass the final checks