This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR
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
HR Hya,2461118.8100,10.65,0.05,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
HR Hya 20260319.3100 10.65CV 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:35:01.79 +02:59:29.9 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_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
V0363 Hya,2461118.8100,11.42,0.05,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
V0363 Hya 20260319.3100 11.42CV 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:11.22 -04:27:48.8 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_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 J084055-0621.5,2461118.8100,11.39,0.05,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 J084055-0621.5 20260319.3100 11.39CV 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:54.58 -06:21:29.8 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_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
WW Hya,2461118.8100,9.21,0.05,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
WW Hya 20260319.3100 9.21CV 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:46.25 -03:16:54.3 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_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
DD Hya,2461118.8100,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DD Hya 20260319.3100 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:31.67 +02:50:06.8 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 13.54 08:06:07.66 +02:35:56.2
219.29159 17.77738 galactic CMi Second-epoch detections are separated by 1.7" and 5.7 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 | 08:06:07.66 +02:35:56.2 (user input) | T | P | (position from user input) SpType: G7 (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,2461118.8100,13.54,0.05,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
target 20260319.3100 13.54CV 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:07.66 +02:35:56.2 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 13.40 08:04:25.16 -06:44:27.9
227.56436 12.89661 galactic Mon Second-epoch detections are separated by 7.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:04:25.16 -06:44:27.9 (user input) | T | P | (position from user input) SpType: G3 (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,2461118.8100,13.40,0.05,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 20260319.3100 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:25.16 -06:44:27.9 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 12.96 08:05:51.99 +02:33:21.9
219.29960 17.69971 galactic CMi Second-epoch detections are separated by 2.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3090999903220823040 | 08:05:52.54 +02:33:18.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (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 3090999903220823040,2461118.8100,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090999903220823040 20260319.3100 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:51.99 +02:33:21.9 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 12.93 08:06:50.48 +02:38:29.5
219.33902 17.95498 galactic CMi Second-epoch detections are separated by 3.4" and 5.0 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 3090995745692409216 | 08:06:50.00 +02:38:31.5 (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 3090995745692409216,2461118.8100,12.93,0.05,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 3090995745692409216 20260319.3100 12.93CV 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:50.48 +02:38:29.5 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 12.91 08:07:40.75 +01:59:16.4
220.04917 17.83517 galactic CMi Second-epoch detections are separated by 0.7" and 5.4 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 | Gaia DR3 3090698293436147456 | 08:07:41.22 +01:59:15.9 (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 3090698293436147456,2461118.8100,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090698293436147456 20260319.3100 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:40.75 +01:59:16.4 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 13.73 08:33:55.08 -03:45:56.3
228.76689 20.73546 galactic Hya Second-epoch detections are separated by 2.2" and 4.8 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 | ATO J128.4761-03.7644 | 08:33:55.08 -03:45:56.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
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
ATO J128.4761-03.7644,2461118.8100,13.73,0.05,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
ATO J128.4761-03.7644 20260319.3100 13.73CV 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:33:55.08 -03:45:56.3 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 11.11 08:11:06.13 -06:53:50.3
228.55900 14.25365 galactic Mon Second-epoch detections are separated by 0.9" and 5.4 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 | Gaia DR3 3063842412688692992 | 08:11:05.98 -06:53:52.1 (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 3063842412688692992,2461118.8100,11.11,0.05,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 3063842412688692992 20260319.3100 11.11CV 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:06.13 -06:53:50.3 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_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: 2461032.87918782 23.12.2025 09:05:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
First image: 2461032.87918782 23.12.2025 09:05:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
Last image: 2461118.81029021 19.03.2026 07:26:39.074 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
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: 5 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): 16622
Objects passed selection criteria: 16607
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: 15403.5
Average stars matched: 15073.8 (97.8593 %)
Memory usage VmPeak: 121464 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 02:34:17 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: 2461032.87918782 23.12.2025 09:05:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
First image: 2461032.87918782 23.12.2025 09:05:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
Last image: 2461118.81029021 19.03.2026 07:26:39.074 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 166
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.43
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: 41 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): 103417
Objects passed selection criteria: 103199
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 92262.8
Average stars matched: 89505.8 (97.0118 %)
Memory usage VmPeak: 2064536 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 02:36:10 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
SExtractor catalog cache: saved Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat to cache
SExtractor catalog cache: saved Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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: 2461118.80975135
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits exists and is non-empty
Saving wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits to local_wcs_cache/
'wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits' -> 'local_wcs_cache/wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits'
wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits exists and is non-empty
Saving wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits to local_wcs_cache/
'wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits' -> 'local_wcs_cache/wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits'
wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
Saving wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits'
wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
Saving wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits to local_wcs_cache/
'wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits' -> 'local_wcs_cache/wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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 08:34:34.300 -02:00:56.07
Second-epoch image center 08:34:14.893 -02:01:08.78
Angular distance between the image centers 0.08 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 08:34:34.300 -02:00:56.07
Second-epoch image center 08:34:12.825 -02:01:08.18
Angular distance between the image centers 0.09 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 08:34:14.893 -02:01:08.78
Second-epoch second image center 08:34:12.825 -02:01:08.18
Angular distance between the image centers 0.00861 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits &> /tmp/tmp.YxVkHUOX86
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits &> /tmp/tmp.6LZHUHpuCI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.HLknq5zucj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.hT5M3F40cS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits and wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits and wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat
Found non-empty wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits and wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat
The reference image (wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits) and catalog (wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat) found
'wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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 8940 out of 17306 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.944981
a=0.000000 b=1.000000 c=22.944981
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
2.1 pix Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
2.5 pix fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
2.5 pix fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
Limiting magnitude estimates:
15.3 mag. Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
15.3 mag. Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
14.8 mag. fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
14.8 mag. fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.0 (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.YxVkHUOX86 (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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits' -> 'wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
WCS-calibrated image found: wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
Checking if the catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
WCS catalog name: wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1389, passed=17306
Got 17306 stars (including 15895 good ones) from the SExtractor catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat
util/solve_plate_with_UCAC5 got 17306 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits -region wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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.6LZHUHpuCI (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-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits' -> 'wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
WCS-calibrated image found: wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
Checking if the catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
WCS catalog name: wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1340, passed=17361
Got 17361 stars (including 15996 good ones) from the SExtractor catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat
util/solve_plate_with_UCAC5 got 17361 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits -region wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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.HLknq5zucj (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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=781, passed=13665
Got 13665 stars (including 12872 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 13665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 927 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.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.hT5M3F40cS (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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=799, passed=13665
Got 13665 stars (including 12857 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 13665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 928 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits'
Saving fully-calibrated image wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits'
Saving fully-calibrated image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits'
Saving fully-calibrated image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits'
Preparing the HTML report for the field Hya-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out01752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21104.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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: 4s
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Considering the candidate 21059_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 21059_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:54:30.38 -02:17:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 0.708 5763904870680466048 133.62657120109 -02.29083145233 11.0798 10.4610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21104_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 21104_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
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Considering the candidate 21107_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 21107_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:03:09.40 +01:40:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 1.868 576737382557951360 135.78865219905 +01.67043148311 10.7677 10.4764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21253_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 21253_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:25:30.72 -05:27:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.176 3065202195038815360 126.37816266670 -05.46120048705 12.0777 11.3457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 05214_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 05214_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01752_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 01752_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10883_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 10883_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:58:16.32 -00:49:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06966_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 06966_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16812_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 16812_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Hya-03-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 ####
08:40:54.58 -06:21:29.8
08:15:11.22 -04:27:48.8
08:57:46.25 -03:16:54.3
08:12:31.67 +02:50:06.8
08:35:01.79 +02:59:29.9
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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
SExtractor catalog cache: saved Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat to cache
SExtractor catalog cache: saved Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
Creating symlink local_wcs_cache/wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits exists and is non-empty
wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits exists and is non-empty
wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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 08:34:34.300 -02:00:56.07
Second-epoch image center 08:34:14.893 -02:01:08.78
Angular distance between the image centers 0.08 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 08:34:34.300 -02:00:56.07
Second-epoch image center 08:34:12.825 -02:01:08.18
Angular distance between the image centers 0.09 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 08:34:14.893 -02:01:08.78
Second-epoch second image center 08:34:12.825 -02:01:08.18
Angular distance between the image centers 0.00861 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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits &> /tmp/tmp.BwJs8pgB28
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits &> /tmp/tmp.g3PjhUpFNz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.pPzGIyUu3Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.Qs4KBdjAbp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits and wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits and wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat
Found non-empty wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits and wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat
The reference image (wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits) and catalog (wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat) found
'wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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 9072 out of 110379 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.836087
a=0.000000 b=1.000000 c=22.836087
From vast_summary.log: estimated ref. image limiting mag.: -7.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 105 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
2.0 pix Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
2.4 pix fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
2.4 pix fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
Limiting magnitude estimates:
15.4 mag. Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
15.4 mag. Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
14.9 mag. fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
14.9 mag. fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.3 (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.BwJs8pgB28 (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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits' -> 'wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
WCS-calibrated image found: wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
Checking if the catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
WCS catalog name: wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=8618, passed=110358
Got 110358 stars (including 101559 good ones) from the SExtractor catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat
util/solve_plate_with_UCAC5 got 110358 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits -region wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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.g3PjhUpFNz (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-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits' -> 'wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
WCS_IMAGE_NAME=wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
WCS-calibrated image found: wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
Checking if the catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits alredy exist and is non-empty...
Catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat corresponding to the image wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
WCS catalog name: wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=8564, passed=109534
Got 109534 stars (including 100784 good ones) from the SExtractor catalog wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat
util/solve_plate_with_UCAC5 got 109534 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits -region wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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.pPzGIyUu3Y (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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=5153, passed=75852
Got 75852 stars (including 70613 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 75852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 922 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: 0.56"
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 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 920 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.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.Qs4KBdjAbp (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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=5109, passed=75861
Got 75861 stars (including 70673 good ones) from the SExtractor catalog wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 75861 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 923 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits
Saving fully-calibrated image wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/wcs_Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits
Saving fully-calibrated image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits
Saving fully-calibrated image wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.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-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits
Preparing the HTML report for the field Hya-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out121015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out127723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129584.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 28s
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: 5s
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Considering the candidate 128723_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128723_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:36:38.91 -06:48:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.220 5755062873048505728 129.16150450476 -06.80539086180 14.4725 13.8136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128731_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128731_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:28:31.65 -02:01:25.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)
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Considering the candidate 128736_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128736_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:38:25.65 -05:52:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 1.505 5755273670043048064 129.60686566052 -05.88141806069 14.5362 13.8931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128744_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128744_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:32:47.25 -06:37:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.672 5754950478047763200 128.19674096623 -06.62590861071 14.4835 14.0008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128745_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128745_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:04:36.31 -03:51:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 3.529 5759529467237203584 136.15220466559 -03.86238778657 14.4643 14.0380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128746_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128746_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:51:29.42 -06:34:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.863 5760150828746032896 132.87273182088 -06.58105001305 14.1120 13.6609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128747_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128747_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:50:09.31 -06:26:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.299 5760167665017876608 132.53878430369 -06.44766629846 14.1260 13.6016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128752_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128752_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:32:32.22 +01:13:07.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)
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Considering the candidate 128754_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128754_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:45:57.78 -05:54:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.337 5760491466896380288 131.49043727671 -05.91340296414 14.3793 13.8714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128755_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128755_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:12:58.33 -01:34:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 4.127 3071183095914810752 123.24212817526 -01.57130680825 14.0788 13.4532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128762_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128762_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:51:07.18 +01:16:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.659 3075622889505757568 132.77982451409 +01.27753620492 14.1268 13.6136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128764_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128764_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:03:45.51 -01:41:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 0.975 5763436444367065216 135.93950928540 -01.69643932790 14.0600 13.6002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128765_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128765_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:05:03.23 -05:07:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.309 3067443725590845568 121.26388572743 -05.11856307051 13.2798 12.7637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128767_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128767_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:49:47.29 -06:58:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.809 5757110988332791424 132.44726232386 -06.97143889603 13.9259 13.5201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128770_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128770_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:06:33.82 -02:44:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.695 3070618771573875456 121.64053214497 -02.74884072691 13.8209 13.2086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128776_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128776_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:56:57.78 -05:07:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.885 5760827573856642688 134.24126817217 -05.12241133859 13.8907 13.1360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128777_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128777_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:13:48.67 -05:59:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.081 3064467588129987328 123.45295300173 -05.99539609157 13.7531 13.1194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128778_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128778_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:47:03.74 -06:10:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.880 5760425122537565056 131.76608416528 -06.18207420147 14.0177 13.5404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128779_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128779_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:54:51.23 -03:15:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.035 5763496638334073216 133.71373628370 -03.25139655928 14.1718 13.7677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128781_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128781_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:07:02.69 +02:50:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 2.734 3091011718673042048 121.76052873646 +02.84260410024 13.3535 12.8634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128785_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128785_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:03:24.93 -04:36:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.978 3068646350792999808 120.85525312514 -04.60221417434 13.2227 12.7291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128789_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128789_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:57:04.75 -00:24:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.797 3074417408149046784 134.26965341090 -00.40308949760 14.0394 13.5509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128791_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128791_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:52:54.22 -05:56:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.871 5760306512720690304 133.22671091830 -05.94966564097 14.0918 13.4660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128794_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128794_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:03:42.36 -05:34:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.793 3067401669270804096 120.92572608140 -05.57784366522 12.9671 12.4965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128795_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128795_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:58:49.30 -05:41:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.272 5757734617584034816 134.70618093775 -05.68821989073 13.9182 13.4816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128796_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128796_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:52:46.12 -04:43:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.224 5761011024796004864 133.19237550448 -04.73160205969 13.6165 13.0118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128798_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128798_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:52:56.02 +00:00:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.075 3074612816277198080 133.23317995402 +00.01605775614 14.0768 13.5955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128799_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128799_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:04:19.09 -05:17:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.992 3067434242302644736 121.08061928586 -05.29561317760 12.9106 12.2499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128801_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128801_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:05:35.02 +02:26:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.391 3090962176228132864 121.39477149279 +02.43318852757 13.0258 12.5952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128803_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128803_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:54:51.26 +01:05:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.210 576831360737527552 133.71352526306 +01.09253284299 13.8786 13.5072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128806_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128806_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:56:31.88 -06:11:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.629 5757595731226450176 134.13269808642 -06.19540115788 13.8323 13.3803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128815_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128815_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:04:29.40 +02:13:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.766 577342942882085248 136.12268389748 +02.21767041630 13.4008 12.7254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128816_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128816_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:03:54.26 +00:53:50.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 128819_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128819_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:04:26.99 -05:41:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.780 3067384519461084928 121.11377463684 -05.69677384923 12.8152 12.2841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128822_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128822_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:03:39.12 -03:16:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.729 5762614421986609792 135.91318586476 -03.27774766723 13.6834 13.2471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128827_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128827_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:06:12.54 +02:16:09.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 128829_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128829_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:05:08.04 -05:27:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.498 3067416615756810240 121.28390836100 -05.45352241520 12.9156 12.3366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128830_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 128830_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
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Considering the candidate 128833_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128833_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:03:49.02 -03:23:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.201 5762564462927118592 135.95422397489 -03.38802172042 13.6772 13.2976 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128836_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128836_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:05:22.72 +02:04:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.460 3090899916382297600 121.34374738519 +02.08010689032 12.7172 12.0669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128839_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 128839_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
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Considering the candidate 128851_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128851_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:59:25.26 +02:53:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.812 578229389771655168 134.85564166226 +02.89504450712 13.4273 12.9468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128861_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 128861_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
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Considering the candidate 128867_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 128867_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
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Considering the candidate 128873_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128873_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:01:53.93 -05:09:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128876_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 128876_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
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Considering the candidate 128877_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128877_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:04:23.51 +02:04:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.830 3084944446009752832 121.09661887076 +02.07720079791 11.9092 11.2559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128878_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128878_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:04:51.11 +02:32:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.438 3090978771981564032 121.21173376970 +02.54409882468 12.0657 11.4644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128881_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128881_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:02:28.16 -04:34:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.731 5759371545584588032 135.61779826089 -04.57212215556 12.5267 12.0306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128892_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128892_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:38:33.54 -05:47:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128939_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 128939_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:03:09.39 +01:40:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 1.736 576737382557951360 135.78865219905 +01.67043148311 10.7677 10.4764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129085_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129085_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:22:32.87 -06:12:06.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129168_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129168_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:13:44.77 -05:44:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129194_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129194_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:11:54.51 -05:20:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.421 3067562335403902208 122.97709334873 -05.34127929945 12.6581 12.3041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129208_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129208_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:20:10.47 -05:20:48.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129228_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129228_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:40:46.79 +02:52:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.282 3079190736018400896 130.19480283042 +02.87179078597 12.9827 12.4809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129255_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129255_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:30:44.67 -06:15:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129299_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129299_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:55:40.78 +00:44:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.331 3074758669070503296 133.92000457585 +00.74900210504 13.1522 12.6561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129317_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129317_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:57:36.99 -05:59:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.305 5757628652150926464 134.40420497816 -05.99233182431 13.1687 12.7237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129330_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129330_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:38:10.66 -01:53:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.655 3073196885819168512 129.54442341226 -01.89895966567 13.2734 12.8345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129339_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129339_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:26:23.93 -02:44:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.237 3066923794025660160 126.59968108624 -02.74720370796 13.1286 12.4460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129350_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129350_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:34:36.61 -00:41:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.589 3073564191421639424 128.65254853059 -00.69760791153 13.2587 12.7848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129354_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129354_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:29:47.79 -06:20:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.833 3064850767930655616 127.44959145620 -06.34219147864 13.2584 12.6919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129358_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129358_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:00:25.87 +01:44:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.991 576940281108215680 135.10767177926 +01.74190450085 13.3289 12.8518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129363_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129363_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:57:31.08 -04:52:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.213 5760838332750805376 134.37975416097 -04.87697239459 13.1949 12.7001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129371_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129371_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:45:22.35 -03:41:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.140 5762153589175789824 131.34310855369 -03.69873302773 13.3409 12.9570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129433_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129433_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:27:32.07 -02:02:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.846 3075994863737696128 126.88377760403 -02.03860081285 13.7809 13.7907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129460_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129460_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:44:41.18 -06:51:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.372 5754181339600491392 131.17189331882 -06.86403017698 13.4673 13.0420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129493_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129493_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:29:46.41 -06:20:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.237 3064850733570918912 127.44329277966 -06.34989373178 13.4278 12.7817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129508_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129508_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:59:31.91 -06:36:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.298 5757370915457874176 134.88332095529 -06.60665691485 13.6183 13.1223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129535_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129535_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:22:11.75 +02:10:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 4.587 3090244366930860928 125.54937670971 +02.17448131000 13.9552 13.4998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129544_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129544_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:45:00.92 -04:53:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129561_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129561_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:42:16.72 -03:55:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.238 5761776731565414784 130.56943243777 -03.93191896410 14.0683 13.4949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129584_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 129584_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
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Considering the candidate 129585_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129585_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:09:17.98 -01:40:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.875 3070858739984189696 122.32450539517 -01.68343470311 13.5595 13.1647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129597_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129597_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:56:06.53 -06:17:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.401 5757593158541239040 134.02745760361 -06.28657803446 13.6736 13.1083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129601_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129601_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:04:10.54 -01:49:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.496 5763419986052385152 136.04460982300 -01.81711365613 13.8082 13.1420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129646_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129646_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:48:50.44 +00:29:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.063 3075428825703469824 132.21018973744 +00.49762215719 13.7499 13.2542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129665_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129665_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:51:08.49 -06:15:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 5.196 5760266174387985664 132.78576814616 -06.25913938583 14.2047 13.7251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129696_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129696_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:53:15.00 -01:15:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.351 3073890054885187712 133.31284511031 -01.25803132540 13.9087 13.2815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129697_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129697_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:30:19.81 +02:51:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 0.858 3079834225198625664 127.58244720931 +02.86057994362 13.8736 13.1938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129707_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129707_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:49:43.15 -06:56:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.332 5760113514070293120 132.42988195978 -06.94660490603 13.7291 13.1446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129720_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129720_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:56:13.84 -01:00:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.178 5764426795106123392 134.05797589716 -01.01619823661 14.4384 13.9847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129735_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129735_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:40:22.35 +02:47:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 2.981 3079188571354889984 130.09376650241 +02.79939214662 14.3043 13.7516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129746_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129746_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:57:57.72 -02:20:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 3.778 5763681979057674240 134.49045869041 -02.33965977495 14.2987 13.7715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129747_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129747_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:58:52.08 -04:37:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.153 5760872722553186560 134.71671537223 -04.62696257754 14.0248 13.5037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129751_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129751_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:50:05.75 +00:22:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.546 3075432055518994304 132.52475649662 +00.37420041454 14.3049 13.7911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129768_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129768_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 09:01:14.38 +01:55:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.196 576949592597288192 135.31024572423 +01.92503678441 13.9881 13.2216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129780_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129780_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:24:05.29 -00:51:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 3.825 3076361280283331968 126.02251521348 -00.85622888493 14.4857 14.1650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129787_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129787_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:25:29.52 -02:07:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.189 3075978100481271296 126.37267105990 -02.12766106269 14.4046 13.9918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129795_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129795_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 129826_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129826_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:26:54.25 -03:53:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 2.019 3066507830737075584 126.72644560289 -03.89175113563 14.2087 13.7172 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129864_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129864_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:28:36.74 +00:45:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.382 3077794081374055296 127.15262956277 +00.76368500791 14.6371 14.1921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129866_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129866_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:51:09.57 -06:56:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 3.770 5757133116004226944 132.79091974926 -06.93884053244 14.4644 13.9217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129875_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129875_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:32:45.24 +00:38:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.657 3077000302697502720 128.18858076986 +00.63374132366 14.8321 14.3626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129988_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 129988_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:50:25.89 -02:28:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.823 5763840751113806464 132.60802211746 -02.47023066406 14.7841 14.2587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 88230_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 88230_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:58:16.32 -00:49:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09711_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 09711_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:40:54.58 -06:21:29.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 73059_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 73059_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:35:01.80 +02:59:29.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 127723_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 127723_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:23:10.38 -01:53:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.767 3070045067018279040 125.79320898624 -01.89054237281 13.8652 12.6373 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121015_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 121015_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:06:12.54 -06:42:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 0.197 3063993217583287680 121.55220552436 -06.70416234743 13.2320 12.6206 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 04331_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
Preparing report for the candidate 04331_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
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Considering the candidate 31686_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 31686_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:15:11.23 -04:27:48.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 73723_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 73723_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks
**** FOUND 08:12:31.64 +02:50:07.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 43696_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022
The candidate 43696_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022 did not pass the final checks