This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G
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,2461119.6585,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1585 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:54:09.45 +06:19:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6585,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1585 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:35.95 +04:53:50.1 ;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-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_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
Gaia DR3 3146242219257322496,2461119.6585,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3146242219257322496 20260320.1585 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:00.90 +08:58:36.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 14.22 08:05:14.73 +01:29:57.3
220.20292 17.06896 galactic CMi Second-epoch detections are separated by 1.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:05:14.73 +01:29:57.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6585,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1585 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:14.73 +01:29:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 13.79 08:03:40.89 +08:44:42.4
213.20088 20.00124 galactic Cnc Second-epoch detections are separated by 7.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:03:40.89 +08:44:42.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6585,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1585 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:40.89 +08:44:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 13.90 08:10:01.88 +09:01:11.6
213.66473 21.53335 galactic Cnc Second-epoch detections are separated by 3.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:10:01.88 +09:01:11.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6585,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1585 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:01.88 +09:01:11.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 13.81 08:05:32.72 +11:03:33.6
211.17618 21.40823 galactic Cnc Second-epoch detections are separated by 2.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:05:32.72 +11:03:33.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6585,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1585 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:32.72 +11:03:33.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 13.36 08:03:46.49 +09:12:56.3
212.76003 20.22610 galactic Cnc Second-epoch detections are separated by 8.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:03:46.49 +09:12:56.3 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6585,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1585 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:46.49 +09:12:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 13.19 08:04:14.04 +08:35:25.1
213.41249 20.05677 galactic Cnc Second-epoch detections are separated by 1.4" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3146196520805379840 | 08:04:13.49 +08:35:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3146196520805379840,2461119.6585,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3146196520805379840 20260320.1585 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:14.04 +08:35:25.1 ;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-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 12.79 08:09:33.62 +10:34:48.4
212.09321 22.09832 galactic Cnc Second-epoch detections are separated by 1.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3146882203743931520 | 08:09:35.59 +10:34:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3146882203743931520,2461119.6585,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3146882203743931520 20260320.1585 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:09:33.62 +10:34:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 12.80 08:04:48.56 +10:52:00.1
211.28151 21.16305 galactic Cnc Second-epoch detections are separated by 4.4" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3147686187261938944 | 08:04:49.09 +10:51:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3147686187261938944,2461119.6585,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3147686187261938944 20260320.1585 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:48.56 +10:52:00.1 ;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-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 12.40 08:07:55.85 +10:33:54.9
211.92431 21.72950 galactic Cnc Second-epoch detections are separated by 0.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3147629596773125504 | 08:07:56.28 +10:33:55.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3147629596773125504,2461119.6585,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3147629596773125504 20260320.1585 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:55.85 +10:33:54.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 12.30 08:05:01.79 +10:15:44.7
211.89227 20.95514 galactic Cnc Second-epoch detections are separated by 1.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3147515900399304960 | 08:05:02.37 +10:15:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3147515900399304960,2461119.6585,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3147515900399304960 20260320.1585 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:01.79 +10:15:44.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_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,2461119.6585,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1585 12.71CV 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-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:22.18 +03:27:33.1 ;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-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1585 2461119.6585 13.11 08:04:26.70 +11:06:53.8
210.99972 21.18702 galactic Cnc Second-epoch detections are separated by 5.0" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3147890795207064960 | 08:04:26.16 +11:06:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3147890795207064960,2461119.6585,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3147890795207064960 20260320.1585 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:26.70 +11:06:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_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,2461119.6585,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1585 13.44CV 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-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:59.77 +04:45:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461119.65873179 20.03.2026 03:48:24.427 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 16268
Objects passed selection criteria: 16257
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: 15580
Average stars matched: 15121.2 (97.0555 %)
Memory usage VmPeak: 120392 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 23:26:05 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461119.65873179 20.03.2026 03:48:24.427 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 573
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: 34 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): 89461
Objects passed selection criteria: 89280
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 84289.2
Average stars matched: 81575 (96.7798 %)
Memory usage VmPeak: 1948028 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 23:27:32 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.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: 2461119.65822301
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
Saving wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits to local_wcs_cache/
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
Saving wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits to local_wcs_cache/
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits'
wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.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 08:34:30.296 +06:00:57.63
Angular distance between the image centers 0.06 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 08:34:31.518 +06:00:45.48
Angular distance between the image centers 0.06 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 08:34:30.296 +06:00:57.63
Second-epoch second image center 08:34:31.518 +06:00:45.48
Angular distance between the image centers 0.00609 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.6FM0IA8S60
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.jB7nh2gbse
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits &> /tmp/tmp.wrYf6ahtLi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits &> /tmp/tmp.qFq5qEnLff
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7589 out of 15650 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955413
a=0.000000 b=1.000000 c=22.955413
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 19 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.3 pix Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.7 pix fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
2.6 pix fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Limiting magnitude estimates:
15.3 mag. Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.3 mag. Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
15.2 mag. fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
15.2 mag. fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6FM0IA8S60 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1186, passed=15650
Got 15650 stars (including 14444 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 15650 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jB7nh2gbse (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=15565
Got 15565 stars (including 14349 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 15565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.wrYf6ahtLi (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=956, passed=15850
Got 15850 stars (including 14875 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat
util/solve_plate_with_UCAC5 got 15850 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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: 0.63"
Estimated accuracy of the plate solution: 0.67"
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-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.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.qFq5qEnLff (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1015, passed=15693
Got 15693 stars (including 14667 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 15693 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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: 0.63"
Estimated accuracy of the plate solution: 0.67"
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-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits'
Preparing the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20796.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20787_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20787_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:35:01.82 +02:59:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20796_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 20796_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 20802_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20802_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:14:19.11 +08:34:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20835_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20835_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:47:06.93 +08:35:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.315 597077763555338624 131.77860819526 +08.59572491313 12.1524 11.7708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20836_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20836_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:47:22.86 +02:18:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.441 3078956707545162496 131.84519929659 +02.31066715676 11.9013 11.1792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20841_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20841_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:57:18.26 +01:30:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.850 576862559379882624 134.32631916049 +01.50837470506 12.2430 11.7275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20846_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20846_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:26:47.13 +05:59:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.590 3093644056884194944 126.69645238291 +05.99103368261 12.1996 11.7490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20860_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20860_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:56:52.26 +09:14:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.472 597450639731702400 134.21733693842 +09.24824692412 12.3660 11.9926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20866_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20866_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:25:23.92 +02:06:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.720 3078198151896544896 126.34904153536 +02.11101021363 12.7398 12.2432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20867_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20867_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:08:24.51 +02:32:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.254 3090941418648347520 122.10181342256 +02.53876021402 12.3841 11.7168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20870_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20870_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:44:55.91 +10:04:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20872_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20872_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:23:42.10 +06:35:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.812 3093925909818026496 125.92555643530 +06.58892773567 12.4451 11.9738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20873_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20873_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:36:26.51 +06:58:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.820 595779278978943616 129.11028404993 +06.98253723987 12.2917 11.8367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20875_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20875_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:33:54.00 +05:49:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.115 594829983831437440 128.47502224808 +05.83089213441 12.3626 11.9241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20877_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20877_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:41:09.49 +06:03:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.994 594676120922984448 130.28926318157 +06.05531310007 12.3140 11.8927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20878_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20878_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 09:00:58.00 +06:38:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.020 583698425032486656 135.24166556511 +06.63663346954 12.3389 11.8517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20880_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20880_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:33:41.61 +08:05:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.166 596468393595405952 128.42332882854 +08.09408990538 12.3423 11.9367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20883_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20883_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:35:53.75 +08:09:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.650 596482073067668992 128.97386720855 +08.15648969771 12.4107 12.1103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20615_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20615_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:13:38.76 +10:11:45.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:54:09.45 +06:19:40.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Creating symlink local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits exists and is non-empty
wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.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 08:34:30.296 +06:00:57.63
Angular distance between the image centers 0.06 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 08:34:31.518 +06:00:45.48
Angular distance between the image centers 0.06 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 08:34:30.296 +06:00:57.63
Second-epoch second image center 08:34:31.518 +06:00:45.48
Angular distance between the image centers 0.00609 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.2wcAH5OULz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.BhRVb2NlnE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits &> /tmp/tmp.n9emEw9CvL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits &> /tmp/tmp.mYwxuLm0gZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7690 out of 90472 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.847783
a=0.000000 b=1.000000 c=22.847783
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 315 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.1 pix Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.5 pix fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
2.4 pix fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Limiting magnitude estimates:
15.5 mag. Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.5 mag. Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
15.3 mag. fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
15.3 mag. fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2wcAH5OULz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6373, passed=90453
Got 90453 stars (including 83928 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 90453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BhRVb2NlnE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6475, passed=90928
Got 90928 stars (including 84300 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 90928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.n9emEw9CvL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=5778, passed=77902
Got 77902 stars (including 72047 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat
util/solve_plate_with_UCAC5 got 77902 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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: 0.57"
Estimated accuracy of the plate solution: 0.60"
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-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.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.mYwxuLm0gZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=6348, passed=80416
Got 80416 stars (including 73984 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 80416 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.59"
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-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-47-40_20.00sec_-14.90C_LIGHT_0118.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_232151_TTUQ2b1x1_12119_DvU3tj7G/wcs_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119.fits
Preparing the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out03728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out107317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107733.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 35s
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: 9s
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Considering the candidate 107253_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107253_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:25:23.17 +02:16:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.434 3090211484661260288 126.34657995998 +02.26674672309 14.4254 14.0198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107263_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107263_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:53:02.43 +07:57:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107274_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107274_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:07:54.80 +10:06:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.521 3146826953284745088 121.97765029453 +10.10769378523 13.8714 13.4010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107277_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107277_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:38:04.32 +07:05:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.341 595408674840454656 129.51769547803 +07.09516214621 14.1810 13.5785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107278_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107278_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:04:19.72 +07:31:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.536 3145780871050689792 121.08231095420 +07.53101377029 14.0182 13.6002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107281_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107281_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:49:24.79 +02:42:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.238 580979818108965248 132.35275649775 +02.71178936827 14.4606 13.9735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107285_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107285_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:05:27.37 +10:12:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 5.125 3147503290375494656 121.36548797336 +10.21314255659 13.6670 13.1866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107286_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107286_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:05:18.53 +05:57:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 4.380 3095887301124668160 121.32829652177 +05.96719447012 13.8226 13.3665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107289_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107289_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:57:04.76 +01:07:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.662 576776556954978176 134.26975608645 +01.13197243790 14.5698 14.1314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107290_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107290_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:06:16.08 +09:25:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.457 3146640379905672576 121.56769012434 +09.43189572702 13.9570 13.5185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107296_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107296_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:04:26.28 +08:18:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.247 3145994313745047552 121.10924234253 +08.30940102036 13.6322 12.9706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107302_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107302_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:42:52.23 +04:33:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.728 582223674997598208 130.71749489251 +04.55962872333 14.1441 13.6542 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 107306_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107306_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 09:00:44.78 +00:57:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.841 576582596231278592 135.18687181877 +00.96186688459 14.4499 14.0361 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107311_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107311_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:09:35.84 +04:15:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.007 3094642207285611008 122.39954861808 +04.26437359912 14.1773 13.7386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107313_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107313_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:05:27.83 +07:18:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 4.306 3097731560081548672 121.36481226745 +07.31351641607 13.7591 13.3466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107317_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107317_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107318_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107318_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107319_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107319_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 09:01:47.20 +08:17:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.248 585120407100050048 135.44673420313 +08.29556709388 13.8077 13.1189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107320_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107320_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107321_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107321_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:08:38.94 +10:14:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 4.175 3146835680658252672 122.16111701531 +10.24812446744 13.4335 12.8846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107323_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107323_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:06:24.33 +08:31:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 2.652 3146015685502390272 121.60210452488 +08.52901737964 13.8017 13.4497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107324_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107324_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107327_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107327_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107329_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107329_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107331_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107331_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107335_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107335_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:04:26.95 +10:24:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.026 3147568058482142976 121.11342778979 +10.41123217661 13.3673 12.9684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107336_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107336_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107338_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107338_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:03:54.04 +09:09:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.096 3146295889168461696 120.97374240929 +09.16172647865 13.0902 12.3373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107341_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107341_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:07:57.97 +10:31:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 5.053 3147629218816008192 121.99280958652 +10.52667311231 13.2036 12.5028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107342_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107342_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:35:30.78 +02:15:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.704 3079518145670212864 128.87826978192 +02.26058348440 13.9050 13.5173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107346_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107346_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:04:16.98 +01:27:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.885 3084838755454913920 121.07084543011 +01.45840822045 13.4973 12.8461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107348_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107348_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 107351_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107351_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107355_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107355_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:19:13.68 +10:01:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.404 600599297437773312 124.80698545101 +10.02241685947 13.6584 13.2829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107356_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107356_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:07:37.90 +08:50:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.390 3146403710027826048 121.90838949297 +08.84519395994 13.3107 12.8073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107359_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107359_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 107361_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107361_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 107363_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107363_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107364_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107364_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:58:29.02 +02:32:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.461 577794120606343040 134.62051395816 +02.53446952148 13.5621 13.0941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107371_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107371_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:06:36.37 +10:16:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.569 3147594824717977728 121.65225861380 +10.26874632715 12.6448 12.1677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107372_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107372_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:04:29.43 +08:38:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.357 3146197208000237824 121.12142104797 +08.64561507736 12.7667 12.2677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107373_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107373_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107376_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107376_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107377_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107377_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107378_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107378_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107379_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107379_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:08:04.76 +10:48:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.398 3147643718625554688 122.02079396414 +10.80910947256 12.0631 11.3277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107380_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107380_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:07:47.72 +09:09:20.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 107381_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107381_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:45:47.89 +04:59:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.833 582344277679189120 131.44905179715 +04.99270060379 12.6719 11.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107386_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107386_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107387_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107387_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:06:55.51 +10:19:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.160 3147596542704870784 121.73177828015 +10.31938966708 11.6582 11.0000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107388_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107388_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107427_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107427_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:54:09.45 +06:19:40.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 107428_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107428_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107438_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107438_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107439_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107439_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107446_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107446_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107468_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107468_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107471_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107471_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107474_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107474_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:57:18.29 +01:30:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.531 576862559379882624 134.32631916049 +01.50837470506 12.2430 11.7275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107477_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107477_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107478_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107478_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107479_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107479_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 107490_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107490_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107497_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107497_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107503_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107503_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 107506_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107506_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107509_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107509_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107519_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107519_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107523_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107523_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107529_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107529_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:29:34.52 +08:55:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107535_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107535_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107538_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107538_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107546_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107546_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 107552_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107552_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107555_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107555_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107566_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107566_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107568_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107568_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:37:49.25 +05:42:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107569_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107569_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107570_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107570_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107573_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107573_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107580_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107580_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107582_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107582_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107587_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107587_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107590_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107590_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107591_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107591_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107596_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107596_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107597_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107597_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107603_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107603_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 107604_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107604_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107608_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107608_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107610_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107610_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107614_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107614_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107616_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107616_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107620_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107620_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:41:12.38 +00:56:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107622_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107622_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107624_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107624_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107628_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107628_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107629_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107629_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107631_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107631_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107632_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107632_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107636_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107636_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107639_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107639_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107641_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107641_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107642_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107642_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107643_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107643_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 107649_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107649_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 107650_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107650_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 107652_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107652_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107653_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107653_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 107655_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107655_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107658_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107658_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107659_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107659_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107663_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107663_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107666_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107666_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107671_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107671_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107676_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107676_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107681_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107681_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107683_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107683_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107684_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107684_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107685_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107685_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107692_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107692_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107699_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107699_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:55:33.48 +05:55:24.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 107700_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107700_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107707_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107707_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107712_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107712_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107713_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107713_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107716_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107716_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107719_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107719_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107721_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107721_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107723_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107723_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107728_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107728_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107730_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107730_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107731_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107731_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107733_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
Preparing report for the candidate 107733_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
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Considering the candidate 107734_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107734_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107738_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107738_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107739_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107739_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:53:38.39 +03:04:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107740_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107740_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107741_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107741_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107742_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107742_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107745_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107745_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107750_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107750_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107751_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107751_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 107752_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107752_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107753_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107753_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107756_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107756_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107762_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107762_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107765_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107765_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 107766_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107766_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107769_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107769_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107772_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107772_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107774_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107774_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107776_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107776_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107779_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107779_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107781_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107781_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107782_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107782_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:29:37.23 +01:22:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.542 3077902829945753856 127.40513972936 +01.37570544094 13.5840 13.0283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107787_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107787_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107788_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107788_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107790_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107790_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107791_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107791_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107792_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107792_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107798_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107798_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 107800_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107800_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107802_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107802_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 107803_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107803_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107812_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107812_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107816_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107816_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107818_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107818_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107821_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107821_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107822_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107822_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 107830_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107830_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107831_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107831_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107834_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107834_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 107839_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107839_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107844_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107844_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107852_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107852_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107853_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107853_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107858_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107858_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 107859_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107859_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107863_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107863_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107864_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107864_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 09:03:45.44 +09:54:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107868_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107868_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107870_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107870_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107871_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107871_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107872_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107872_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107874_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107874_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107875_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107875_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107877_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107877_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107878_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107878_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107886_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107886_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107888_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107888_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107890_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107890_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107895_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107895_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 107896_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107896_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107897_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107897_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 107901_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107901_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107903_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107903_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:10:37.05 +03:49:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 3.572 3091544642511268352 122.65463694068 +03.83348506933 14.2842 13.9345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107906_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107906_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107909_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107909_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107910_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107910_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:22:12.66 +02:27:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107913_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107913_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107915_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107915_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:16:06.32 +03:46:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107916_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107916_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107917_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107917_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107920_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107920_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107923_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107923_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107925_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107925_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107928_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107928_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107929_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107929_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107934_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107934_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107935_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107935_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107937_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107937_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107938_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107938_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107939_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107939_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107942_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107942_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107944_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107944_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107947_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107947_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107949_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107949_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107951_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107951_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107955_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107955_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 107958_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107958_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107963_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107963_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 107968_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107968_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107969_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107969_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 107970_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107970_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107972_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107972_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 107976_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107976_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107979_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107979_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:30:50.13 +02:17:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.706 3079657169466926464 127.70909910913 +02.28983417164 14.2891 13.7999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107980_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107980_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 107985_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107985_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 107987_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107987_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 107988_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107988_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 107989_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107989_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 107990_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 107990_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 108007_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108007_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108008_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108008_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 108010_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108010_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:07:15.97 +02:45:51.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)
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Considering the candidate 108011_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108011_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108013_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108013_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108014_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108014_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:49:29.97 +00:53:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.387 3075513586882914304 132.37497245770 +00.89876747394 14.1560 13.5667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108015_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108015_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108017_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108017_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 108025_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108025_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:30:03.48 +01:30:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 2.748 3077906025401383808 127.51449783347 +01.50167993757 14.6343 14.2111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108028_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108028_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 108030_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108030_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108031_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108031_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108032_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108032_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108033_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108033_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 09:01:14.51 +01:55:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108035_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108035_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108036_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108036_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108038_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108038_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108041_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108041_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108043_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108043_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 108044_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108044_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 108045_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108045_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108047_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108047_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108049_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108049_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108050_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108050_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 108051_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108051_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108052_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108052_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108054_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108054_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108056_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108056_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108057_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108057_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 108061_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108061_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108071_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108071_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 108072_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108072_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 108073_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108073_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108075_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108075_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108078_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108078_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 108081_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108081_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108083_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108083_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108084_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108084_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 108086_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108086_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 108090_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108090_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 108091_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108091_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108092_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108092_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:11:02.50 +02:36:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.189 3090840130435259776 122.76038460884 +02.61668982605 14.5316 14.1299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108094_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108094_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 09:02:40.75 +00:47:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 4.785 576609225028727680 135.67099993928 +00.79886230709 14.7093 14.1507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108095_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108095_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 108098_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108098_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108100_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108100_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 108101_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108101_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108107_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108107_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 108112_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108112_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108113_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108113_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 108115_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108115_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108116_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108116_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108118_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108118_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 108121_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108121_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 108122_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108122_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 108123_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108123_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 09:01:17.21 +08:49:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.654 585367380604105344 135.32182024037 +08.82516517496 14.3522 13.7896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108125_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108125_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108126_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108126_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108128_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108128_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 108130_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108130_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 108131_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108131_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:14:06.75 +04:00:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 2.734 3091653631601219968 123.52859005930 +04.01676782217 14.7037 14.2381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108134_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108134_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 108137_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108137_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 108149_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108149_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 108151_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108151_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108154_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108154_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:22:03.75 +05:24:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.213 3093330867869711360 125.51475593323 +05.40355278482 14.4867 14.0162 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108160_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108160_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108163_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108163_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 108165_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108165_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 108171_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108171_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 108192_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108192_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 108232_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108232_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 108249_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 108249_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 105142_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 105142_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 06217_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 06217_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:04:46.74 +10:19:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20546_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 20546_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:14:19.11 +08:34:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78550_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 78550_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:35:01.82 +02:59:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02295_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 02295_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 47134_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 47134_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 07583_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 07583_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks
**** FOUND 08:13:38.75 +10:11:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03728_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119
The candidate 03728_fd_Hya-01-Q2b1x1_2026-03-19_22-48-24_20.00sec_-15.00C_LIGHT_0119 did not pass the final checks