This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7497,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2497 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:53:52.12 +06:41:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7497,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2497 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:07.52 +03:37:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7497,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2497 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:56.42 +04:53:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7497,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2497 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:21.17 +05:16:40.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2497 2461121.7497 14.56 08:46:05.89 +10:47:39.4
216.13137 30.31551 galactic Cnc Second-epoch detections are separated by 2.0" and 6.7 pix This object is listed in tocp_transients_list.txt 2.4" TCP J08460573+1047397 2026-03-21.1936 14.5mag
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 | 08:46:05.89 +10:47:39.4 (user input) | T | P | (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
target,2461121.7497,14.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2497 14.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:46:05.89 +10:47:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VW Cnc,2461121.7497,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VW Cnc 20260322.2497 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:38.44 +10:11:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_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
TSVSC1 TN-N221313303-64-67-2,2461121.7497,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N221313303-64-67-2 20260322.2497 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:48.98 +03:34:11.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TV Cnc,2461121.7497,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TV Cnc 20260322.2497 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:18.86 +08:34:22.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461121.74993898 22.03.2026 05:59:44.728 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 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): 15594
Objects passed selection criteria: 15587
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 15161.5
Average stars matched: 14859.8 (98.0098 %)
Memory usage VmPeak: 120076 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 01:45:56 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461121.74993898 22.03.2026 05:59:44.728 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 120
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 46 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): 90483
Objects passed selection criteria: 90318
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 87675
Average stars matched: 84788.8 (96.708 %)
Memory usage VmPeak: 1886392 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 01:47:42 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.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: 2461121.74937144
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
Saving wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits to local_wcs_cache/
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
Saving wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits to local_wcs_cache/
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits'
wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:17.935 +06:00:02.24
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:15.240 +05:59:52.57
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:34:17.935 +06:00:02.24
Second-epoch second image center 08:34:15.240 +05:59:52.57
Angular distance between the image centers 0.01149 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.urnBcpSaDL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.IMq1huCHYU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits &> /tmp/tmp.WMtBwWb9gK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits &> /tmp/tmp.rYkKRW8ELF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7589 out of 15650 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955413
a=0.000000 b=1.000000 c=22.955413
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.3 pix Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.2 pix fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
2.2 pix fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Limiting magnitude estimates:
15.3 mag. Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.3 mag. Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
15.2 mag. fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
15.2 mag. fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.urnBcpSaDL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1186, passed=15650
Got 15650 stars (including 14444 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 15650 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IMq1huCHYU (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=15565
Got 15565 stars (including 14349 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 15565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WMtBwWb9gK (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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1071, passed=14974
Got 14974 stars (including 13870 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat
util/solve_plate_with_UCAC5 got 14974 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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits -region wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.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.rYkKRW8ELF (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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1053, passed=14897
Got 14897 stars (including 13816 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 14897 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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits -region wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
Saving fully-calibrated image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits'
Preparing the HTML report for the field Hya-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20772.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20756_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 20756_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:26:33.87 +03:30:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.100 3091860404209463168 126.64097668793 +03.51135058617 12.6231 12.5348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20769_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 20769_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:35:01.81 +02:59:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20772_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
Preparing report for the candidate 20772_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20774_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 20774_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:14:18.84 +08:34:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 2.080 3098353608785731968 123.57820118281 +08.57349649149 11.2013 9.7247 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20785_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 20785_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:56:52.22 +09:14:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20788_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 20788_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:52:11.41 +04:28:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20791_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 20791_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:36:26.50 +06:58:56.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20614_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 20614_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:13:38.42 +10:11:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 4.753 648603356632052224 123.40931122447 +10.19724638046 10.7595 9.5376 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Hya-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:53:52.12 +06:41:02.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Creating symlink local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits exists and is non-empty
wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:17.935 +06:00:02.24
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:15.240 +05:59:52.57
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:34:17.935 +06:00:02.24
Second-epoch second image center 08:34:15.240 +05:59:52.57
Angular distance between the image centers 0.01149 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.iVcTpZqv8Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.Z5zRbeGA0i
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits &> /tmp/tmp.Gw3lDoabck
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits &> /tmp/tmp.1k9Rcf3DMT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7690 out of 90472 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.847783
a=0.000000 b=1.000000 c=22.847783
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 99 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.1 pix Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.2 pix fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
2.2 pix fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Limiting magnitude estimates:
15.5 mag. Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.5 mag. Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
15.4 mag. fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
15.4 mag. fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.iVcTpZqv8Y (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6373, passed=90453
Got 90453 stars (including 83928 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 90453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Z5zRbeGA0i (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6475, passed=90928
Got 90928 stars (including 84300 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 90928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Gw3lDoabck (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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=5767, passed=85618
Got 85618 stars (including 79723 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat
util/solve_plate_with_UCAC5 got 85618 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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits -region wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.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.1k9Rcf3DMT (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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=5782, passed=85846
Got 85846 stars (including 79919 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 85846 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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits -region wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Saving fully-calibrated image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-58-55_20.00sec_-14.90C_LIGHT_0089.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.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_2026-03-22_CI_Hya-01-Q1b1x1_010026_TTUQ1b1x1_24262_H6MuyNHt/wcs_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090.fits
Preparing the HTML report for the field Hya-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out107254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83192.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 107254_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107254_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:30:02.38 +10:29:09.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)
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Considering the candidate 107255_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107255_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:23:58.19 +03:06:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.728 3092005406601717376 125.99290969749 +03.11530414391 14.8338 14.0241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107263_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107263_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:26:44.25 +03:00:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.927 3091779388242208256 126.68395625313 +03.01366732070 14.6844 14.0342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107265_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107265_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:24:57.26 +06:02:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 1.404 3093753870608220160 126.23857850028 +06.04475121571 14.8923 14.3746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107266_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107266_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:05:00.04 +08:39:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 1.513 3146010428462271232 121.25056261855 +08.65254110167 14.8556 14.3077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107268_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107268_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:33:45.50 +09:23:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 2.833 599755147384619008 128.44006496000 +09.39629395722 14.8379 14.3203 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 107270_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107270_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:23:19.42 +01:55:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 3.347 3090178018276111104 125.83109005604 +01.92421901356 14.7512 14.2902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107272_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107272_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:49:24.78 +02:42:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107273_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107273_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:10:53.99 +10:36:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107274_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107274_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:38:43.56 +00:59:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107279_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107279_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:04:50.10 +02:06:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107282_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107282_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:18:27.05 +10:37:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107285_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107285_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:16:27.27 +04:05:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.796 3091623017074548352 124.11365270721 +04.09824724582 14.0749 13.6493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107290_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107290_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:02:24.65 +03:07:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107308_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107308_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:53:52.12 +06:41:02.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 107343_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
Preparing report for the candidate 107343_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
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Considering the candidate 107415_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107415_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:53:38.48 +03:04:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107459_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
Preparing report for the candidate 107459_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
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Considering the candidate 107534_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107534_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:22:12.69 +02:27:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107552_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107552_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:10:37.12 +03:49:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107599_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107599_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:03:33.02 +05:41:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107613_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
Preparing report for the candidate 107613_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
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Considering the candidate 107626_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107626_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:22:03.78 +05:24:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107648_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107648_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:57:02.33 +03:50:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 3.089 578545224486872192 134.26015371596 +03.84678967911 14.9162 14.3596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107664_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107664_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:03:53.26 +05:07:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 3.668 580238571177337344 135.97123082359 +05.13325614963 14.9677 14.4597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107679_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
Preparing report for the candidate 107679_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
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Considering the candidate 107704_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107704_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:50:34.93 +05:28:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.279 582717012120961280 132.64511408403 +05.47616306639 15.0183 14.4985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107706_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107706_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:21:32.72 +02:12:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.726 3090248146502094336 125.38615932368 +02.20900222444 14.9381 14.3305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107721_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107721_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:22:35.09 +10:32:28.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)
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Considering the candidate 107727_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107727_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:53:42.04 +01:29:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 2.566 577607886529402624 133.42501208240 +01.49735968051 14.9348 14.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107747_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107747_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:15:35.97 +07:38:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 1.218 3097942975551072640 123.89956089216 +07.64649330555 15.3642 14.8623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107748_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107748_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:50:19.03 +02:46:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 2.506 581000498376194176 132.57930090074 +02.77238740241 14.9202 14.4869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107757_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107757_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:57:13.18 +02:06:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.816 577753816633304704 134.30505108512 +02.10301592300 14.9175 14.4095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107760_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107760_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:01:44.18 +01:22:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 2.064 576702202480612608 135.43353180205 +01.37026810756 14.9239 14.2418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107763_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107763_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:59:35.04 +01:30:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.061 576904478260865024 134.89607425968 +01.50781308752 14.8767 14.3612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107766_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107766_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:33:46.90 +01:42:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107767_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107767_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:23:13.70 +09:57:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.388 600378501758440832 125.80718989077 +09.95213555216 15.0499 14.6189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107768_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107768_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:10:09.32 +08:37:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.471 3146337773690077952 122.53872534391 +08.63218689226 14.9131 14.4211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107785_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107785_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:09:03.82 +02:11:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 1.564 3090731622382276864 122.26600947266 +02.18789665442 14.7194 14.2971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107789_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107789_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:33:06.15 +09:48:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 2.019 599786998861940736 128.27507115979 +09.81415705579 14.9937 14.3409 NOT_AVAILABLE#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 107791_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107791_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:11:02.39 +02:36:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107802_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107802_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:04:21.77 +01:28:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 3.785 577046865016321920 136.08965882293 +01.47651152459 14.7894 14.3357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107811_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107811_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:08:38.69 +05:19:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 3.399 3095039027904439296 122.16074039498 +05.33071016590 14.6823 14.2134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107814_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107814_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:02:59.58 +05:30:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.182 583360295142705536 135.74800153196 +05.51163276867 14.6456 14.0851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107816_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107816_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:12:39.00 +05:16:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 3.932 3096313877275374080 123.16227997550 +05.28162554789 14.8057 14.2893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107825_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107825_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:18:09.76 +02:19:46.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)
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Considering the candidate 107831_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107831_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:10:38.55 +01:54:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 4.302 3090658814096925824 122.65989685829 +01.90367007118 14.9669 14.5639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107836_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107836_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:25:12.41 +02:04:11.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)
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Considering the candidate 107842_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107842_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:53:06.84 +07:11:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.904 584673489983259648 133.27797021556 +07.19588591662 14.8468 14.3352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107847_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107847_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:58:01.74 +01:30:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 2.046 576860360356604288 134.50699655265 +01.50478654849 14.7996 14.3679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107860_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107860_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:18:29.68 +10:35:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 0.330 648676130558079104 124.62357505801 +10.59253811026 14.7894 14.1006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107875_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107875_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:19:50.81 +01:14:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 2.000 3089661037357627264 124.96136575562 +01.24115967692 14.6046 13.9131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107877_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107877_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:03:20.78 +03:48:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.066 578405998826884608 135.83632201409 +03.80689019643 14.7784 14.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107880_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107880_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:12:40.25 +09:51:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 3.525 3146586950512482304 123.16725746544 +09.85131711272 14.2109 13.1303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107886_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107886_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:06:48.90 +03:19:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.833 3094128804075229312 121.70352200974 +03.31670795298 14.9303 14.5245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107889_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107889_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:46:05.40 +09:24:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.820 598023279131608448 131.52255313801 +09.41047491774 14.9252 14.3988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107890_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107890_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:47:07.47 +02:25:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 2.297 3078970829397626624 131.78089171933 +02.41792727880 14.7474 14.2187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107895_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107895_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:52:02.32 +01:56:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.198 577871189499534336 133.00980566141 +01.94155884194 14.6219 13.8350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107902_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107902_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:55:17.20 +06:44:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 2.664 584409572833044480 133.82201880033 +06.74726333335 15.0726 14.5655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107903_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107903_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:04:58.90 +10:10:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.583 591600928634172032 136.24507458087 +10.18281070036 14.9801 14.2560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107911_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107911_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:59:39.00 +01:20:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.947 576887882507242496 134.91233808330 +01.33968276637 15.0110 14.5735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107913_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107913_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:11:18.19 +07:52:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.585 3097825018570148352 122.82557160093 +07.87677138125 14.7337 14.3387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107915_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107915_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:04:38.11 +09:55:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 2.053 3147465803900969344 121.15828001961 +09.91987779337 14.9949 14.4723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107916_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107916_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:51:29.11 +01:38:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.372 3075673363961273088 132.87130636915 +01.63604755875 15.0253 14.4099 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 107919_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107919_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:37:32.91 +00:59:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 2.324 3078343974626151040 129.38648184179 +00.99314040124 14.7551 14.0447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107931_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107931_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:00:49.08 +05:50:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.730 583433069068532608 135.20406924519 +05.83449534217 15.0291 14.4031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107932_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107932_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 09:03:50.34 +02:55:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 0.556 577536078971319936 135.95990472624 +02.91841271426 14.5883 13.5397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107937_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107937_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:08:51.45 +03:22:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 3.202 3091148268570417152 122.21387644154 +03.38176485243 14.7636 14.3359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107939_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107939_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:12:44.60 +01:39:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 3.730 3089885960500920064 123.18555437895 +01.66085891253 14.9211 14.4798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107942_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107942_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:47:59.71 +04:43:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.376 582276692073969408 131.99842767149 +04.71926827786 14.9671 14.5080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107943_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107943_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:14:46.50 +06:58:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.938 3096780482522179584 123.69386769087 +06.97530339406 14.9162 14.5173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107947_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107947_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:49:26.43 +01:47:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 2.552 3075875708460453632 132.35942333915 +01.79232571712 14.8675 14.3747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107948_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107948_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:53:49.92 +03:39:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.821 581156530243304320 133.45809475188 +03.65638585198 15.1143 14.6218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107957_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107957_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:36:17.76 +01:49:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 2.724 3078718117817192064 129.07381846370 +01.83012353317 14.8389 14.1645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107964_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107964_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:09:49.38 +04:51:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 1.469 3094772568132038016 122.45548450279 +04.85061632272 14.7551 14.2862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107978_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107978_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:19:27.18 +01:19:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 2.442 3089674991706734336 124.86317736860 +01.32247995699 14.6302 13.9936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107983_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107983_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:21:17.60 +03:00:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 2.631 3090513953438497792 125.32307946468 +03.00570334079 15.0173 14.6425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107985_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107985_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:29:25.18 +01:02:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.933 3077817239837525120 127.35491188346 +01.03470350183 15.0034 14.4896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107987_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107987_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:52:45.12 +02:27:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.153 577930868070190720 133.18768828792 +02.45186970073 14.8501 14.3058 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 107996_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 107996_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:34:57.56 +05:54:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.636 594790405708160512 128.73981830978 +05.91212091949 15.1034 14.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108002_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108002_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:42:57.29 +02:35:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.214 3079203208603548032 130.73842677730 +02.58943590002 14.8552 14.3031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108009_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108009_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:08:26.08 +06:14:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 2.044 3097372810053170432 122.10812078987 +06.23736046280 15.0634 14.6435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108026_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108026_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:26:52.68 +10:49:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 2.252 600901491336184576 126.71903362014 +10.81632400769 15.3136 14.8822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108028_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108028_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:38:12.82 +02:30:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 1.739 3079151394118005248 129.55373693552 +02.50758408398 14.8747 14.3701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108030_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108030_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:16:31.55 +03:57:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.902 3091616454364416640 124.13123787414 +03.95976880853 15.2104 14.7003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108032_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108032_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:05:39.23 +02:52:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.499 3094012152763670656 121.41309320406 +02.87939557314 14.8900 14.5869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108035_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108035_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:26:54.03 +08:58:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 2.306 599455874063705344 126.72546539800 +08.97087861955 15.1909 14.7397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108037_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108037_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:24:47.95 +10:08:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.859 600746288398116736 126.19973297017 +10.14648548334 14.9535 14.4776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108044_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108044_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:15:58.53 +05:18:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.321 3096278246226754304 123.99353300423 +05.30449794367 15.0163 14.4585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108049_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108049_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:26:11.64 +08:10:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 2.121 599112414118760448 126.54804619136 +08.17302015902 14.9769 14.4923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108085_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108085_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:10:17.03 +03:29:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.596 3091528287275908864 122.57093586541 +03.49696965036 14.8198 14.2937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108093_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108093_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:22:31.16 +01:54:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 2.004 3090096237804338816 125.62948953107 +01.90704918171 14.7260 14.0454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108107_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108107_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:09:49.64 +03:55:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 2.497 3094550913461109504 122.45676967380 +03.91746837380 14.9122 14.4075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108109_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108109_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:10:24.62 +08:17:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 5.179 3098272004406828160 122.60353691911 +08.29728050131 14.6703 13.7831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108143_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 108143_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks
**** FOUND 08:09:44.86 +07:41:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=15.00, MAG_FAINT_SEARCH_LIMIT=15.98)GAIADR2_OUTPUT=# 0.599 3097803612453385984 122.43693028971 +07.69916574804 14.8803 14.4276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07583_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
Preparing report for the candidate 07583_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
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Considering the candidate 83192_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
Preparing report for the candidate 83192_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
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Considering the candidate 78550_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090
The candidate 78550_fd_Hya-01-Q1b1x1_2026-03-22_00-59-44_20.00sec_-14.90C_LIGHT_0090 did not pass the final checks