This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 25.2561* 09 35 21.22 +07 54 47.2 12.6 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,2461124.7561,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2561 12.62CV 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-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:35:21.22 +07:54:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20_00sec_-15_00C_LIGHT_0033_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20_00sec_-14_90C_LIGHT_0032_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-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20_00sec_-15_00C_LIGHT_0033_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20_00sec_-14_90C_LIGHT_0032_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,2461124.7561,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2561 13.91CV 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-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:35:57.86 +03:31:51.1 ;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-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20_00sec_-15_00C_LIGHT_0033_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20_00sec_-14_90C_LIGHT_0032_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-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20_00sec_-15_00C_LIGHT_0033_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20_00sec_-14_90C_LIGHT_0032_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,2461124.7561,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2561 14.32CV 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-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:13:01.00 +08:42:03.4 ;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-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20_00sec_-15_00C_LIGHT_0033_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20_00sec_-14_90C_LIGHT_0032_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-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20_00sec_-15_00C_LIGHT_0033_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20_00sec_-14_90C_LIGHT_0032_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 03 25.2561* 09 36 02.65 +08 01 47.5 14.8 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,2461124.7561,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2561 14.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:36:02.65 +08:01:47.5 ;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-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20_00sec_-15_00C_LIGHT_0033_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20_00sec_-14_90C_LIGHT_0032_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-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20_00sec_-15_00C_LIGHT_0033_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20_00sec_-14_90C_LIGHT_0032_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: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461124.75637100 25.03.2026 06:09:00.454 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8566
Objects passed selection criteria: 8538
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 6437.25
Average stars matched: 6123 (95.1183 %)
Memory usage VmPeak: 114368 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:18:04 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461124.75637100 25.03.2026 06:09:00.454 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 47
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 16 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): 47933
Objects passed selection criteria: 47810
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 38390
Average stars matched: 36340.2 (94.6607 %)
Memory usage VmPeak: 147352 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:18:51 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.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: 2461124.75582513
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits'
wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:26:00.402 +05:59:51.30
Angular distance between the image centers 0.07 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:26:00.278 +05:59:30.07
Angular distance between the image centers 0.07 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 09:26:00.402 +05:59:51.30
Second-epoch second image center 09:26:00.278 +05:59:30.07
Angular distance between the image centers 0.00592 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.7M5Gepor50
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.Uzk5fzXILa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits &> /tmp/tmp.9K3aVqEoJU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.IRm6TsEqTu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat' -> 'wcsmag.cat'
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 5047 out of 9705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.925124
a=0.000000 b=1.000000 c=22.925124
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.4 pix fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
2.3 pix fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Limiting magnitude estimates:
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
14.5 mag. fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
14.5 mag. fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.7M5Gepor50 (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_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=629, passed=9705
Got 9705 stars (including 9071 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 9705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Uzk5fzXILa (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_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=616, passed=9704
Got 9704 stars (including 9075 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 9704 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 937 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9K3aVqEoJU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=326, passed=5600
Got 5600 stars (including 5269 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 5600 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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: 0.51"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.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.IRm6TsEqTu (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=333, passed=5596
Got 5596 stars (including 5257 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 5596 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 932 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-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits'
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:26:00.402 +05:59:51.30
Angular distance between the image centers 0.07 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:26:00.278 +05:59:30.07
Angular distance between the image centers 0.07 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 09:26:00.402 +05:59:51.30
Second-epoch second image center 09:26:00.278 +05:59:30.07
Angular distance between the image centers 0.00592 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.ZTXSouKezK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.2w3Mf35yzI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits &> /tmp/tmp.SYB854DEH0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.RfE5U9y1zZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat' -> 'wcsmag.cat'
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 5088 out of 52265 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.799339
a=0.000000 b=1.000000 c=22.799339
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.2 pix fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
2.1 pix fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Limiting magnitude estimates:
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
14.7 mag. fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
14.7 mag. fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZTXSouKezK (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_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=3222, passed=52238
Got 52238 stars (including 48939 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 52238 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2w3Mf35yzI (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_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3213, passed=52136
Got 52136 stars (including 48850 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 52136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SYB854DEH0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1376, passed=33508
Got 33508 stars (including 32084 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 33508 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.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.RfE5U9y1zZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1371, passed=33884
Got 33884 stars (including 32462 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 33884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-08-13_20.00sec_-14.90C_LIGHT_0032.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_011552_TTUQ2b1x1_2600_sfhY2UDf/wcs_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033.fits
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out65572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out66831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70048.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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65572_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65572_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:32:54.00 +04:22:34.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65573_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65573_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:47:45.06 +04:08:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.005 3848044170388615680 146.93801527677 +04.14291133429 14.2083 13.6489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65581_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65581_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:04:28.24 +02:12:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.278 577342942882085888 136.11766502495 +02.21436723684 13.5751 13.0719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65582_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65582_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:18:43.44 +06:27:00.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65584_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65584_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:47:37.51 +05:37:02.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65585_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65585_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:06:37.40 +02:50:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.321 577487219423400448 136.65614808409 +02.84913354123 13.1100 12.6822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65586_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65586_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:29:31.43 +07:43:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.461 586496544686691200 142.38136151892 +07.71856767326 13.1573 12.4612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65588_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65588_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:36:24.77 +02:47:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65589_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65589_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:02:39.88 +05:37:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.624 583365032490850176 135.66685531006 +05.62064069688 12.3932 11.7207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65590_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 65590_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:34:04.68 +02:30:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.467 3850580297037430400 143.51962609002 +02.51169121641 11.7424 11.3221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66549_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 66549_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:51:27.36 +08:48:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.494 3878742393302602752 147.86405258308 +08.80528964214 12.2253 11.7962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66831_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
Preparing report for the candidate 66831_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67076_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 67076_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:39:33.06 +03:55:12.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67120_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 67120_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:09:02.51 +07:29:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.880 584039381011870208 137.26067038895 +07.48691825190 12.7261 12.1383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67140_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 67140_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:37:19.02 +06:51:32.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67279_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 67279_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:10:45.03 +06:21:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.992 580848770066513664 137.68790223189 +06.36563206430 12.8084 12.3112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67349_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 67349_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:04:12.96 +06:41:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.668 583877924601172096 136.05417942881 +06.69612778721 12.8456 12.3403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67405_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 67405_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67588_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 67588_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:51:22.35 +08:35:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.881 3878734426138064896 147.84328593044 +08.58564723408 13.0797 12.4106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67952_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 67952_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:09:49.97 +10:12:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.150 591757158069052288 137.45855465329 +10.21537940569 13.3600 12.8183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68010_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 68010_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:37:17.45 +06:48:25.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68067_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 68067_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:14:28.57 +07:47:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.017 587109354915283328 138.61925719141 +07.79012078387 13.5673 13.0706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68314_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 68314_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68353_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 68353_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:23:44.55 +05:14:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.582 585508500345303808 140.93599271682 +05.23382644338 13.6960 13.1534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68426_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 68426_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:15:16.49 +09:45:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68508_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 68508_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:19:23.67 +10:10:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68839_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 68839_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68841_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 68841_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68969_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
Preparing report for the candidate 68969_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69040_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 69040_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:11:58.20 +03:07:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.288 578774090408539136 137.99281628469 +03.13097094682 13.6442 13.0446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69168_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 69168_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:21:19.61 +05:31:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.105 585568217570537216 140.33228691233 +05.52379594210 14.2368 13.6605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69303_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 69303_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks
**** FOUND 09:23:34.66 +05:13:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.580 585508049373159808 140.89425705692 +05.21755340073 14.3333 13.8173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69434_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
Preparing report for the candidate 69434_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69824_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033
The candidate 69824_fd_Hya-02-Q2b1x1_2026-03-25_01-09-00_20.00sec_-15.00C_LIGHT_0033 did not pass the final checks