This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8151,11.26,0.05,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 20260319.3151 11.26CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:54:18.42 +06:10:54.4 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_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
VW Cnc,2461118.8151,11.38,0.05,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
VW Cnc 20260319.3151 11.38CV 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-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:38.65 +10:11:45.5 ;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-01-Q2b1x1_2025-12-23_03-18-58_20_00sec_-15_00C_LIGHT_0483_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20_00sec_-15_00C_LIGHT_0483_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20_00sec_-15_00C_LIGHT_0483_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20_00sec_-15_00C_LIGHT_0483_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 14.12 08:05:19.72 +11:01:32.5
211.18480 21.34583 galactic Cnc Second-epoch detections are separated by 4.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:05:19.72 +11:01:32.5 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 14.12CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:19.72 +11:01:32.5 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 13.97 08:07:07.09 +09:46:10.7
212.60547 21.20876 galactic Cnc Second-epoch detections are separated by 4.0" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:07:07.09 +09:46:10.7 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 13.97CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:07.09 +09:46:10.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_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
target,2461118.8151,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 13.79CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:36.00 +10:15:09.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 13.65 08:04:24.56 +07:44:15.6
214.24784 19.72235 galactic Cnc Second-epoch detections are separated by 2.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:04:24.56 +07:44:15.6 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 13.65CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:24.56 +07:44:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 12.94 08:04:18.14 +09:15:39.4
212.77648 20.36306 galactic Cnc Second-epoch detections are separated by 0.6" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3146302898555059968 | 08:04:18.58 +09:15:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3146302898555059968,2461118.8151,12.94,0.05,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
Gaia DR3 3146302898555059968 20260319.3151 12.94CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:18.14 +09:15:39.4 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 12.60 08:04:41.77 +09:57:26.3
212.14981 20.75041 galactic Cnc Second-epoch detections are separated by 6.7" and 0.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3147469171155327360 | 08:04:41.31 +09:57:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3147469171155327360,2461118.8151,12.60,0.05,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
Gaia DR3 3147469171155327360 20260319.3151 12.60CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:41.77 +09:57:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_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
ASAS J080418+0137.2,2461118.8151,11.29,0.05,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
ASAS J080418+0137.2 20260319.3151 11.29CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:18.94 +01:37:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_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,2461118.8151,12.59,0.05,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 20260319.3151 12.59CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:30.03 +03:23:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_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,2461118.8151,12.94,0.05,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 20260319.3151 12.94CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:41:02.90 +04:41:39.4 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_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,2461118.8151,14.41,0.05,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 20260319.3151 14.41CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:28.59 +05:01:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 12.77 08:03:49.87 +01:34:29.3
219.96000 16.79213 galactic CMi Second-epoch detections are separated by 2.8" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3084852327551323008 | 08:03:49.68 +01:34:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3084852327551323008,2461118.8151,12.77,0.05,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
Gaia DR3 3084852327551323008 20260319.3151 12.77CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:49.87 +01:34:29.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_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
TV Cnc,2461118.8151,11.54,0.05,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
TV Cnc 20260319.3151 11.54CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:19.03 +08:34:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 13.08 09:01:52.71 +08:05:24.2
220.98839 32.61759 galactic Cnc Second-epoch detections are separated by 1.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:01:52.71 +08:05:24.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.574+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 13.08CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:52.71 +08:05:24.2 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_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: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461118.81535703 19.03.2026 07:33:56.847 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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: 4 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): 14987
Objects passed selection criteria: 14972
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 13911.2
Average stars matched: 13673.2 (98.2892 %)
Memory usage VmPeak: 120068 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:58:11 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: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461118.81535703 19.03.2026 07:33:56.847 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 429
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 30 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): 85800
Objects passed selection criteria: 85654
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 77731.5
Average stars matched: 75635.5 (97.3035 %)
Memory usage VmPeak: 2569248 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:59:36 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.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: 2461118.81484414
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
Saving wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits to local_wcs_cache/
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
Saving wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits to local_wcs_cache/
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits'
wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:22.316 +06:00:06.32
Angular distance between the image centers 0.03 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:21.564 +06:00:08.07
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:34:22.316 +06:00:06.32
Second-epoch second image center 08:34:21.564 +06:00:08.07
Angular distance between the image centers 0.00315 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.harrI8nebk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.i8uL1BkBxJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits &> /tmp/tmp.RsIdHGMN2e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits &> /tmp/tmp.P3xFVaclNc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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 7589 out of 15650 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955413
a=0.000000 b=1.000000 c=22.955413
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.3 pix Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.5 pix fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
2.5 pix fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
Limiting magnitude estimates:
15.3 mag. Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.3 mag. Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
14.9 mag. fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
14.9 mag. fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.harrI8nebk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1186, passed=15650
Got 15650 stars (including 14444 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 15650 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.i8uL1BkBxJ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=15565
Got 15565 stars (including 14349 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 15565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.RsIdHGMN2e (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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=741, passed=12484
Got 12484 stars (including 11733 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat
util/solve_plate_with_UCAC5 got 12484 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.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.P3xFVaclNc (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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=736, passed=12351
Got 12351 stars (including 11600 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 12351 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits'
Preparing the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20804.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: 1s
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Considering the candidate 20778_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 20778_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:05:11.30 +10:49:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.24, MAG_FAINT_SEARCH_LIMIT=11.22)GAIADR2_OUTPUT=# 1.938 603671195485488640 136.29753696438 +10.83302456886 9.8912 9.1885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20790_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 20790_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:35:01.80 +02:59:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20804_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 20804_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20812_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 20812_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:14:19.02 +08:34:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.230 3098353608785731968 123.57820118281 +08.57349649149 11.2013 9.7247 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20823_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 20823_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:05:17.56 +10:43:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 0.723 591659649426970112 136.32329895763 +10.72920882569 11.4844 11.0713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20830_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 20830_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:15:51.39 +01:45:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.463 3089946158762370816 123.96411962497 +01.75210081681 11.5857 10.7656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20853_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 20853_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:05:55.06 +10:35:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.224 591652395226762112 136.47945223053 +10.58669044799 11.9529 11.5292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20888_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 20888_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:44:55.89 +10:04:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.542 598314134316703104 131.23296487878 +10.06895503677 12.3829 11.9413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11989_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 11989_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:12:31.74 +02:50:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20614_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 20614_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Hya-01-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 ####
08:13:38.65 +10:11:45.5
08:54:18.42 +06:10:54.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Creating symlink local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits exists and is non-empty
wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:22.316 +06:00:06.32
Angular distance between the image centers 0.03 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:21.564 +06:00:08.07
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:34:22.316 +06:00:06.32
Second-epoch second image center 08:34:21.564 +06:00:08.07
Angular distance between the image centers 0.00315 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.37qzXGNRLG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.84gT15Nak8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits &> /tmp/tmp.PZU1hnLPF8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits &> /tmp/tmp.S36wJLMndF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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 7690 out of 90472 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.847783
a=0.000000 b=1.000000 c=22.847783
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 281 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.1 pix Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.4 pix fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
2.4 pix fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
Limiting magnitude estimates:
15.5 mag. Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.5 mag. Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
15.0 mag. fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
15.0 mag. fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.37qzXGNRLG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6373, passed=90453
Got 90453 stars (including 83928 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 90453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.84gT15Nak8 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6475, passed=90928
Got 90928 stars (including 84300 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 90928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.PZU1hnLPF8 (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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=4127, passed=65633
Got 65633 stars (including 61447 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat
util/solve_plate_with_UCAC5 got 65633 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.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.S36wJLMndF (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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=4222, passed=66119
Got 66119 stars (including 61823 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 66119 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.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_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits
Preparing the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out03509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out04244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out06217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out107248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67194.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 33s
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: 7s
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Considering the candidate 107225_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107225_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:53:02.48 +07:57:37.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)
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Considering the candidate 107239_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107239_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:13:42.29 +11:03:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 4.843 648869782043297152 123.42484513356 +11.06244606070 13.8424 13.3275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107240_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107240_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:38:43.55 +00:59:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.159 3078423066447977856 129.68113733696 +00.99310752619 14.4232 13.9688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107241_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107241_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:36:32.53 +02:12:12.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)
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Considering the candidate 107242_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107242_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:09:49.90 +10:19:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 4.041 3146857499092253696 122.45844436883 +10.32168965858 13.5502 13.0522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107247_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107247_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107248_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107248_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107250_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107250_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:22:43.84 +08:49:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 2.735 599392033669808000 125.68222125774 +08.81750801872 13.8077 13.3239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107253_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107253_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:10:44.79 +09:23:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 2.116 3146540152549010176 122.68616533782 +09.39432070329 13.4669 12.8516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107256_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107256_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:09:00.14 +10:59:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 2.211 649650607097484416 122.25075357465 +11.00034090816 13.8119 13.3692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107262_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107262_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:07:03.65 +10:42:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.694 3147647807434464768 121.76568145535 +10.70428807619 13.2557 12.6204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107263_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107263_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:05:00.24 +07:33:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.841 3145800834058652928 121.25079314437 +07.55844530901 13.2894 12.6425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107266_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107266_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:05:49.04 +10:33:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.068 3147618532937264000 121.45491006657 +10.55093566554 13.2914 12.8206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107267_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107267_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:01:00.32 +09:54:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.160 603495067466402944 135.25101428876 +09.91604041571 13.9952 13.5219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107268_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107268_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:03:55.54 +11:00:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.130 3147882553167221376 120.98200028381 +11.00618493011 12.9955 12.3559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107269_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107269_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 107271_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107271_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107275_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107275_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:06:29.55 +10:46:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.391 3147628943937932800 121.62351331890 +10.77827251516 13.2562 12.7111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107276_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107276_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107282_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107282_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:03:37.45 +07:53:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 0.645 584297663165002880 135.90615766491 +07.88955404315 13.5786 12.8824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107283_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107283_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:27:20.47 +04:47:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.324 3092657416996391296 126.83518315817 +04.79624039584 13.8431 13.2359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107284_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107284_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:04:16.91 +01:52:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.624 3084885897015623936 121.07138363430 +01.87289745531 13.0381 12.5529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107287_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107287_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:50:39.88 +03:13:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.841 581124266448960384 132.66620940946 +03.22867633579 14.0861 13.5678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107288_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107288_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:07:21.00 +10:07:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.867 3146838291998698496 121.83606140948 +10.11988987951 12.9286 12.2470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107296_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107296_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107297_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107297_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 107300_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107300_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:06:08.61 +10:03:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.213 3146746444120076288 121.53704746643 +10.05619771784 12.6270 11.9686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107303_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107303_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:07:39.39 +10:58:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.139 3147661585689326336 121.91368635831 +10.97404823265 12.6435 12.1603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107307_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107307_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:01:02.60 +10:20:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.291 603548836161412224 135.26076058482 +10.33609333509 13.4344 12.9913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107316_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107316_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:38:33.63 +01:38:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.677 3078672655587880832 129.64009388810 +01.63371311975 13.0857 12.6219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107324_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107324_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:10:33.87 +11:03:39.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 107325_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107325_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 107326_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107326_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107327_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107327_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 107332_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107332_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107383_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107383_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:54:18.41 +06:10:54.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 107386_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107386_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107410_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107410_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107416_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107416_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107424_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107424_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107432_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107432_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 107457_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107457_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107458_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107458_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 107468_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107468_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:29:34.49 +08:55:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.512 599631074369191936 127.39374781440 +08.91685898485 12.6256 12.2224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107474_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107474_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 107485_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107485_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 107499_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107499_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107502_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107502_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107506_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107506_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107507_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107507_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:37:49.24 +05:42:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.522 594595860869425792 129.45510732631 +05.71332700174 12.5998 11.9675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107515_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107515_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 107518_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107518_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:04:26.17 +11:06:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.745 3147890795207064960 121.10898342126 +11.11631604859 12.4471 11.8363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107521_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107521_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107529_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107529_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107533_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107533_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107536_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107536_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107537_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107537_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107538_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107538_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 107539_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107539_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:20:27.54 +09:25:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.822 600241578201185920 125.11467961402 +09.42391198605 12.8089 12.3267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107544_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107544_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107553_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107553_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107560_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107560_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:25:01.33 +04:27:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 0.275 3092272003811380096 126.25548769539 +04.46119574484 12.8044 12.1613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107561_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107561_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:06:14.46 +05:35:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.954 3095809098360368000 121.56070308139 +05.59321894043 12.8850 12.4731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107562_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 107562_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 107563_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107563_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107568_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107568_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107570_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107570_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107574_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107574_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107576_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107576_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107577_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107577_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 107585_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107585_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 107586_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107586_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:41:12.38 +00:56:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.197 3078367025716053376 130.30153043726 +00.93951452919 12.8756 12.4443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107590_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107590_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107592_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107592_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107594_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107594_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107601_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107601_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107604_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107604_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 107606_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107606_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107607_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107607_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107613_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107613_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107615_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107615_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107617_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107617_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107620_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107620_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107623_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107623_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107628_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107628_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107635_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107635_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 107639_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107639_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107640_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107640_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 107642_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107642_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 107646_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107646_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:11:45.96 +04:15:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.446 3094587266064380416 122.94143089969 +04.26620261917 13.3031 12.9873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107647_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107647_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:36:08.59 +02:02:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.461 3078737595493834624 129.03589679665 +02.03442676585 13.2735 12.8442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107653_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107653_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:55:33.36 +05:55:25.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 107654_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107654_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 107661_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107661_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 107662_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107662_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107663_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107663_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107666_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107666_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 107667_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107667_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107668_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107668_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:53:38.17 +03:04:35.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 107669_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107669_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107671_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107671_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:18:44.87 +01:57:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.988 3090134999883431168 124.68677085416 +01.96550602438 13.3973 12.9897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107673_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107673_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:14:05.52 +01:07:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.254 3089796208567895936 123.52359334347 +01.12118905046 13.4880 12.8182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107674_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107674_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 107675_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107675_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107679_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107679_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107681_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107681_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107682_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107682_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:09:28.53 +05:55:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.909 3095097576898499200 122.36866005506 +05.91905988145 13.3087 12.8661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107683_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107683_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107685_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107685_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107690_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107690_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 107699_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107699_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107704_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107704_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107705_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107705_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107706_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107706_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107708_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107708_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:13:02.02 +04:52:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.923 3094737074522398976 123.25866389466 +04.88131769112 13.5154 12.9585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107710_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107710_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107713_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107713_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:55:19.01 +05:59:28.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 107714_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107714_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:05:04.44 +01:20:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.529 3084645481926221568 121.26780120011 +01.34592588144 12.9124 12.2911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107722_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107722_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 107724_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107724_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 107725_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107725_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 107727_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107727_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107731_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107731_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107732_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107732_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:17:45.18 +09:08:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.228 600391249222310016 124.43881967062 +09.14529728446 13.5700 13.1515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107733_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107733_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 107734_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107734_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107735_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107735_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107739_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107739_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107742_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107742_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107744_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107744_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107751_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107751_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107754_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107754_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107757_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107757_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107758_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107758_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107759_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107759_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 107761_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107761_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 107766_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107766_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 107768_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107768_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107769_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107769_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107772_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107772_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107779_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107779_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:23:55.36 +05:08:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.174 3093109900392081152 125.98127024546 +05.14196916938 13.6898 13.0391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107780_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107780_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:35:47.53 +09:52:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.804 599799437087406080 128.94755331948 +09.87930379481 14.0312 13.5305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107781_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107781_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107788_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107788_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 107791_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107791_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107795_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107795_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107798_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107798_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 107799_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107799_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107803_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107803_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107809_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107809_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107810_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107810_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107811_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107811_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107813_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107813_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 107815_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107815_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107816_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107816_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:16:41.45 +07:24:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.242 3097173248691453824 124.17269742136 +07.40945587156 13.7838 13.2197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107818_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107818_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107823_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107823_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107824_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107824_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:25:10.33 +01:10:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.562 3077977734175213824 126.29298463646 +01.17233989198 13.9913 13.5438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107826_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107826_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107827_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107827_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 107829_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107829_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107830_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107830_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107835_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107835_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107846_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107846_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107847_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107847_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107848_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107848_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 107853_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107853_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:33:54.82 +01:34:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.286 3078622838262630528 128.47882614059 +01.56709776964 13.9196 13.2209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107858_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107858_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 107862_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107862_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107863_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107863_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107865_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107865_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107870_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107870_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107871_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107871_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107875_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107875_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:38:12.56 +03:34:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.407 3080130062546031872 129.55240400181 +03.57432824758 13.9919 13.5681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107882_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107882_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107883_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107883_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:16:06.21 +03:46:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 4.619 3091401976581401600 124.02664325287 +03.77977677028 14.2263 13.7183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107886_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107886_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 107889_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107889_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:22:12.60 +02:27:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.602 3090270549051342336 125.55291632787 +02.46306319202 14.0844 13.6306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107891_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107891_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 107895_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107895_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 107898_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107898_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:03:45.43 +09:54:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.410 591496818626805248 135.93939013361 +09.90463462894 14.0077 13.4518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107900_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107900_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107907_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107907_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107910_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107910_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107912_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107912_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 107913_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107913_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107915_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107915_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107921_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107921_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107926_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107926_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107927_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107927_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107930_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107930_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 107932_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107932_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 107933_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107933_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107936_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107936_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107937_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107937_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107940_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107940_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107941_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107941_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107946_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107946_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 107949_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107949_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 107953_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107953_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107956_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107956_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107957_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107957_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 107958_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107958_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107960_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107960_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107961_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107961_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 107962_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107962_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107964_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107964_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 107968_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107968_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 107970_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107970_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 107971_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107971_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107977_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107977_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107978_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107978_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 107979_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107979_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 107980_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107980_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107982_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107982_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 107985_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107985_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 107987_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107987_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 107989_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107989_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107994_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107994_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 107995_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107995_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 107999_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 107999_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 108002_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108002_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 108006_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108006_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 108008_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108008_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 108009_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108009_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 108011_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108011_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 108013_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108013_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 108016_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108016_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 108020_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108020_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 108021_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108021_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 108023_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108023_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 108025_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108025_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 108026_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108026_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 108028_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108028_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 108029_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108029_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 108033_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108033_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:28:21.50 +06:46:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 4.715 595900534495980800 127.09085886987 +06.77766690025 14.2781 13.2588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108035_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108035_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 108036_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108036_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 108037_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 108037_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 108038_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108038_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 108041_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108041_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 108044_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108044_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 108046_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108046_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 108047_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108047_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 108052_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108052_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 108056_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108056_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 108058_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108058_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 108059_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108059_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 108062_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108062_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 108064_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108064_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 108067_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108067_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 108069_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108069_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 108070_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108070_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 108074_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108074_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 108078_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108078_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 108079_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108079_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 108080_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108080_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 108085_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108085_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 108098_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108098_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 108103_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108103_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 108105_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108105_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 108126_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108126_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 108128_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108128_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 108134_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108134_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 108137_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108137_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 108142_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108142_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 108188_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 108188_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 06217_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 06217_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:04:46.82 +10:19:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.751 3147519576891308672 121.19599748694 +10.31997081706 12.4697 12.0184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 04244_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 04244_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:04:03.26 +10:38:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.119 603663327105418368 136.01406917058 +10.64873311692 12.4673 11.7593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84872_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 84872_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 81655_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 81655_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 03509_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 03509_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 09:00:48.74 +10:45:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.543 603712839488385024 135.20293088326 +10.76176089755 13.6381 13.1938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78550_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 78550_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:35:01.80 +02:59:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67194_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 67194_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 33741_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 33741_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 20546_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 20546_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 44885_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 44885_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 101209_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 101209_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 25044_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
Preparing report for the candidate 25044_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
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Considering the candidate 77596_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 77596_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks
**** FOUND 08:12:31.74 +02:50:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07583_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030
The candidate 07583_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030 did not pass the final checks