This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.7245,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.2245 12.43CV 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-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:18.54 +02:07:16.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20_00sec_-14_90C_LIGHT_0211_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!
TCP 2026 02 12.2245* 09 49 19.75 +08 32 08.8 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.7245,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.2245 13.40CV 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-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:49:19.75 +08:32:08.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20_00sec_-14_90C_LIGHT_0211_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,2461083.7245,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.2245 13.51CV 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-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:35:16.53 +04:27:54.9 ;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-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20_00sec_-14_90C_LIGHT_0211_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,2461083.7245,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.2245 13.88CV 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-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:29:01.47 +01:43:45.7 ;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-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20_00sec_-14_90C_LIGHT_0211_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: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
First image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Last image: 2461083.72473928 12.02.2026 05:23:27.474 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8209
Objects passed selection criteria: 8206
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: 7965
Average stars matched: 7592 (95.317 %)
Memory usage VmPeak: 113960 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 23:30:23 CST 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: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
First image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Last image: 2461083.72473928 12.02.2026 05:23:27.474 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 214
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
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: 17 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): 52177
Objects passed selection criteria: 52038
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: 50556.8
Average stars matched: 47979.5 (94.9023 %)
Memory usage VmPeak: 151924 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 23:31:26 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.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: 2461083.72424014
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-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
Saving wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits to local_wcs_cache/
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
Saving wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits to local_wcs_cache/
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits'
wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.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 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:34.453 +05:59:45.29
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:37.397 +05:59:13.15
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:34.453 +05:59:45.29
Second-epoch second image center 09:25:37.397 +05:59:13.15
Angular distance between the image centers 0.01512 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.4gDLEgOlfA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.Uz0BvoiMU5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits &> /tmp/tmp.DrQZ34gk3h
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits &> /tmp/tmp.m25IKxaTy0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
The reference image (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits) and catalog (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat) found
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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 4890 out of 7575 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.831362
a=0.000000 b=1.000000 c=22.831362
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
2.0 pix Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
2.0 pix fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
2.0 pix fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Limiting magnitude estimates:
15.1 mag. Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
15.1 mag. Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
15.2 mag. fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
15.2 mag. fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.1 (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.4gDLEgOlfA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=564, passed=7575
Got 7575 stars (including 6996 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 7575 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 935 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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.Uz0BvoiMU5 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=571, passed=7669
Got 7669 stars (including 7088 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 7669 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 937 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 934 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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.DrQZ34gk3h (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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=624, passed=8512
Got 8512 stars (including 7875 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat
util/solve_plate_with_UCAC5 got 8512 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 937 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: 0.32"
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 937 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: 0.31"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.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.m25IKxaTy0 (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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=638, passed=8351
Got 8351 stars (including 7702 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat
util/solve_plate_with_UCAC5 got 8351 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 934 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 931 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.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_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits'
Preparing the HTML report for the field Hya-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20517_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 20517_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:08:59.24 +09:35:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20521_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 20521_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 08:55:32.84 +06:09:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20522_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 20522_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:22:31.73 +06:19:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20524_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 20524_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:22:27.49 +03:29:35.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20525_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 20525_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:25:46.03 +05:17:03.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Hya-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits exists and is non-empty
wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.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 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:34.453 +05:59:45.29
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:37.397 +05:59:13.15
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:34.453 +05:59:45.29
Second-epoch second image center 09:25:37.397 +05:59:13.15
Angular distance between the image centers 0.01512 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.buUa0bq8fn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.tgp2HeY1Dm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits &> /tmp/tmp.FJJtW6Lz8G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits &> /tmp/tmp.ZeYFMmN61n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
The reference image (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits) and catalog (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat) found
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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 5118 out of 48659 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.698635
a=0.000000 b=1.000000 c=22.698635
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 40 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
1.9 pix Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
1.9 pix fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
1.8 pix fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Limiting magnitude estimates:
15.2 mag. Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
15.2 mag. Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
15.4 mag. fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
15.4 mag. fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.buUa0bq8fn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2287, passed=48648
Got 48648 stars (including 46264 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 48648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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.tgp2HeY1Dm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2205, passed=48320
Got 48320 stars (including 46022 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 48320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 937 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: 0.32"
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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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.FJJtW6Lz8G (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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2570, passed=52966
Got 52966 stars (including 50302 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat
util/solve_plate_with_UCAC5 got 52966 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 932 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 932 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: 0.31"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.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.ZeYFMmN61n (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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2562, passed=53612
Got 53612 stars (including 50943 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat
util/solve_plate_with_UCAC5 got 53612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.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_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-22-44_20.00sec_-14.90C_LIGHT_0211.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.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_2026-02-11_CI_Hya-02-Q1b1x1_232615_TTUQ1b1x1_27077_3X0rV2ql/wcs_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212.fits
Preparing the HTML report for the field Hya-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53487.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 53357_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53357_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 08:58:04.64 +02:57:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53359_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53359_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:22:15.50 +03:16:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53360_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53360_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 08:56:58.22 +09:52:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53368_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53368_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:29:14.84 +03:20:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53370_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53370_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 08:57:32.02 +05:02:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53401_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53401_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:46:33.79 +01:42:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53407_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 53407_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 53422_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53422_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:10:45.04 +06:21:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53424_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53424_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:41:16.77 +04:41:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53454_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 53454_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 53458_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53458_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:12:01.79 +09:44:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.528 590918612949673216 138.00813428208 +09.74936107885 13.4047 12.6066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53459_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 53459_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 53460_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53460_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:47:46.23 +10:05:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.432 3879145609127232512 146.94298552426 +10.09554054160 13.4352 12.7544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53476_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53476_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:53:40.73 +01:34:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53478_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53478_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:07:04.71 +01:26:08.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53487_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 53487_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 53492_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53492_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:02:01.24 +05:05:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53518_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53518_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:15:51.50 +09:00:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53537_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53537_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:50:53.42 +11:05:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53541_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53541_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:26:05.68 +05:10:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53542_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53542_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:03:20.63 +02:32:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 3.495 577413586504074368 135.83683295098 +02.53525669188 14.7587 14.1145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53556_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53556_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:55:29.66 +02:58:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53567_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53567_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:01:05.12 +05:50:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53573_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53573_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:00:19.20 +03:30:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53577_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53577_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:53:08.86 +01:12:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53578_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53578_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:53:15.83 +01:19:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.327 3834644211727490304 148.31657332257 +01.33077314505 14.5490 14.0514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53582_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53582_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:53:19.42 +01:00:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.660 3834561993168699904 148.33143698089 +01.00719746510 14.7153 14.1469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53584_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53584_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:46:00.97 +09:14:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 2.358 3855057194854908800 146.50441062995 +09.24367786608 14.0818 12.7604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53593_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53593_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:51:16.51 +03:09:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53596_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53596_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:48:48.55 +08:58:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53603_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53603_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:52:11.39 +01:05:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53606_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53606_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:53:07.70 +10:26:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 2.254 3879589433867687680 148.28264928906 +10.44859210006 14.6512 14.1413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53609_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53609_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:53:24.08 +04:33:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53623_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53623_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:56:33.86 +02:46:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.425 3848354541905350144 149.14147466430 +02.77479860706 14.4930 13.8942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53631_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53631_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 08:55:30.96 +05:26:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53632_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53632_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:50:18.71 +02:55:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.038 3847140646708590464 147.57868616025 +02.92223802925 13.0773 11.5948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53662_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53662_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:52:36.12 +09:52:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53680_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 53680_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 08:55:12.32 +01:17:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38235_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 38235_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 09:08:59.25 +09:35:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50567_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212
The candidate 50567_fd_Hya-02-Q1b1x1_2026-02-11_23-23-27_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks