This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 42 48.88 +19 31 30.7 7.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,7.46,0.05,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 20260320.1161 7.46CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:48.88 +19:31:30.7 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 04 11 22.63 +22 01 00.7 11.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,11.47,0.05,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 20260320.1161 11.47CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:11:22.63 +22:01:00.7 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 13.87 03:09:11.83 +25:59:24.8
157.85632 -27.38337 galactic Ari Second-epoch detections are separated by 2.4" and 2.8 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 | 03:09:11.83 +25:59:24.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 09 11.83 +25 59 24.8 13.9 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6161,13.87,0.05,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 20260320.1161 13.87CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:09:11.83 +25:59:24.8 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 13.54 03:11:12.24 +26:49:12.8
157.74230 -26.44502 galactic Ari Second-epoch detections are separated by 2.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 112561716916550784 | 03:11:12.75 +26:49:12.8 (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!
TCP 2026 03 20.1161* 03 11 12.24 +26 49 12.8 13.5 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 112561716916550784,2461119.6161,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 112561716916550784 20260320.1161 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:12.24 +26:49:12.8 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 13.11 03:11:29.27 +26:41:49.9
157.87880 -26.51000 galactic Ari Second-epoch detections are separated by 5.1" and 3.7 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 | Gaia DR3 112555566523481088 | 03:11:28.62 +26:41:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 11 29.27 +26 41 49.9 13.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 112555566523481088,2461119.6161,13.11,0.05,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 112555566523481088 20260320.1161 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:29.27 +26:41:49.9 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 12.80 03:08:40.31 +25:08:27.1
158.29122 -28.14976 galactic Ari Second-epoch detections are separated by 0.6" and 3.1 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 111740519169977088 | 03:08:40.84 +25:08:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (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!
TCP 2026 03 20.1161* 03 08 40.31 +25 08 27.1 12.8 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 111740519169977088,2461119.6161,12.80,0.05,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 111740519169977088 20260320.1161 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:40.31 +25:08:27.1 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 42 48.87 +19 31 30.6 7.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,7.75,0.05,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 20260320.1161 7.75CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:48.87 +19:31:30.6 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 04 13 46.42 +26 11 23.0 12.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1161 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:13:46.42 +26:11:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 31 57.36 +23 29 12.1 12.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,12.79,0.05,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
VARIABLE_NAME 20260320.1161 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:31:57.36 +23:29:12.1 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 40 29.99 +16 57 36.3 12.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,12.78,0.05,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 20260320.1161 12.78CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:29.99 +16:57:36.3 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 13.52 03:08:35.76 +26:50:09.4
157.19565 -26.76104 galactic Ari Second-epoch detections are separated by 0.8" and 3.2 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 | 03:08:35.76 +26:50:09.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 08 35.76 +26 50 09.4 13.5 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6161,13.52,0.05,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 20260320.1161 13.52CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:35.76 +26:50:09.4 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 41 15.58 +20 20 23.1 13.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1161 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:15.58 +20:20:23.1 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 13.38 03:08:58.48 +26:48:11.6
157.29449 -26.74060 galactic Ari Second-epoch detections are separated by 8.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:08:58.48 +26:48:11.6 (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!
TCP 2026 03 20.1161* 03 08 58.48 +26 48 11.6 13.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6161,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1161 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:58.48 +26:48:11.6 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 46 09.81 +21 23 15.7 13.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1161 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:09.81 +21:23:15.7 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 23 22.33 +24 15 24.7 14.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,14.06,0.05,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 20260320.1161 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:22.33 +24:15:24.7 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 51 43.96 +19 22 10.9 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1161 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:43.96 +19:22:10.9 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 20 12.43 +18 48 02.0 14.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,14.45,0.05,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 20260320.1161 14.45CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:12.43 +18:48:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 13.34 03:09:33.75 +26:55:33.6
157.33828 -26.56531 galactic Ari Second-epoch detections are separated by 4.8" 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 115557297690459520 | 03:09:34.29 +26:55:34.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (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!
TCP 2026 03 20.1161* 03 09 33.75 +26 55 33.6 13.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 115557297690459520,2461119.6161,13.34,0.05,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 115557297690459520 20260320.1161 13.34CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:09:33.75 +26:55:33.6 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 04 03 14.03 +22 31 31.2 12.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6161,12.92,0.05,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 20260320.1161 12.92CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:03:14.03 +22:31:31.2 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 12.81 04:05:26.91 +16:56:12.9
175.50728 -25.54878 galactic Tau Second-epoch detections are separated by 0.8" 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 | target | 04:05:26.91 +16:56:12.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.681+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 04 05 26.91 +16 56 12.9 12.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6161,12.81,0.05,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 20260320.1161 12.81CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:26.91 +16:56:12.9 ;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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1161 2461119.6161 13.28 03:18:10.70 +26:37:21.0
159.28262 -25.70320 galactic Ari Second-epoch detections are separated by 1.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:18:10.70 +26:37:21.0 (user input) | T | P | (position from user input) J-Ks=0.620+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1161* 03 18 10.70 +26 37 21.0 13.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6161,13.28,0.05,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 20260320.1161 13.28CV 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:18:10.70 +26:37:21.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20_00sec_-14_90C_LIGHT_0058_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: 2461032.75582700 23.12.2025 06:08:13.453 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
First image: 2461032.75582700 23.12.2025 06:08:13.453 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
Last image: 2461119.61635547 20.03.2026 02:47:23.113 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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): 10849
Objects passed selection criteria: 10833
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: 10068.8
Average stars matched: 9898.5 (98.3091 %)
Memory usage VmPeak: 116572 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 22:19:48 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: 2461032.75582700 23.12.2025 06:08:13.453 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
First image: 2461032.75582700 23.12.2025 06:08:13.453 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
Last image: 2461119.61635547 20.03.2026 02:47:23.113 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 647
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
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: 22 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): 65282
Objects passed selection criteria: 65154
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 59381
Average stars matched: 57618.5 (97.0319 %)
Memory usage VmPeak: 164272 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 22:20:59 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
SExtractor catalog cache: saved Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat to cache
SExtractor catalog cache: saved Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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: 2461119.61583075
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits exists and is non-empty
Saving wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits to local_wcs_cache/
'wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits' -> 'local_wcs_cache/wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits'
wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits exists and is non-empty
Saving wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits to local_wcs_cache/
'wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits' -> 'local_wcs_cache/wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits'
wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits exists and is non-empty
Saving wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits to local_wcs_cache/
'wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits' -> 'local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits'
wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits exists and is non-empty
Saving wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits to local_wcs_cache/
'wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits' -> 'local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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 03:41:32.410 +22:00:13.69
Second-epoch image center 03:41:54.740 +21:57:19.91
Angular distance between the image centers 0.10 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 03:41:32.410 +22:00:13.69
Second-epoch image center 03:41:56.044 +21:57:26.23
Angular distance between the image centers 0.10 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 03:41:54.740 +21:57:19.91
Second-epoch second image center 03:41:56.044 +21:57:26.23
Angular distance between the image centers 0.00534 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits &> /tmp/tmp.g7mTQ5AMeE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits &> /tmp/tmp.8taFvbjKCE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits &> /tmp/tmp.l7fTtiMcwE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits &> /tmp/tmp.JcDG0f8Cdh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits and wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits and wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat
Found non-empty wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits and wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat
The reference image (wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits) and catalog (wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat) found
'wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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 5159 out of 11471 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.937799
a=0.000000 b=1.000000 c=22.937799
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
2.0 pix Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
2.4 pix fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
2.4 pix fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
Limiting magnitude estimates:
15.4 mag. Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
15.4 mag. Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
14.9 mag. fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
14.9 mag. fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.g7mTQ5AMeE (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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits' -> 'wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=838, passed=11471
Got 11471 stars (including 10616 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat
util/solve_plate_with_UCAC5 got 11471 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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits -region wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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.8taFvbjKCE (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/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits' -> 'wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=863, passed=11417
Got 11417 stars (including 10531 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat
util/solve_plate_with_UCAC5 got 11417 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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits -region wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.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.l7fTtiMcwE (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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=538, passed=8801
Got 8801 stars (including 8255 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 8801 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 964 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits -region wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.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.JcDG0f8Cdh (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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=7, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=557, passed=8856
Got 8856 stars (including 8288 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 8856 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 965 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: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits -region wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits'
Saving fully-calibrated image wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits'
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits'
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits'
Preparing the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20635.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20610_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 20610_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20620_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 20620_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:45:09.76 +24:29:03.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20635_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 20635_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20644_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 20644_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:36:48.22 +19:41:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20649_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 20649_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:42:07.77 +22:51:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.276 65027591568709504 055.53275790240 +22.86031254431 12.3874 11.7919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:11:22.63 +22:01:00.7
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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
SExtractor catalog cache: saved Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat to cache
SExtractor catalog cache: saved Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
Creating symlink local_wcs_cache/wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits exists and is non-empty
wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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 03:41:32.410 +22:00:13.69
Second-epoch image center 03:41:54.740 +21:57:19.91
Angular distance between the image centers 0.10 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 03:41:32.410 +22:00:13.69
Second-epoch image center 03:41:56.044 +21:57:26.23
Angular distance between the image centers 0.10 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 03:41:54.740 +21:57:19.91
Second-epoch second image center 03:41:56.044 +21:57:26.23
Angular distance between the image centers 0.00534 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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits &> /tmp/tmp.wHr87OqKXz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits &> /tmp/tmp.cH0N5UXAvL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits &> /tmp/tmp.zq7UhLYAH8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits &> /tmp/tmp.zh2ZDuwQ4f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits and wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits and wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat
Found non-empty wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits and wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat
The reference image (wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits) and catalog (wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat) found
'wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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 5202 out of 69004 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.817299
a=0.000000 b=1.000000 c=22.817299
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 389 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
2.0 pix Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
2.3 pix fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
2.3 pix fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
Limiting magnitude estimates:
15.6 mag. Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
15.6 mag. Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
15.1 mag. fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
15.0 mag. fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.5 (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.wHr87OqKXz (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/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits' -> 'wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=4109, passed=68990
Got 68990 stars (including 64762 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat
util/solve_plate_with_UCAC5 got 68990 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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits -region wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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.cH0N5UXAvL (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/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits' -> 'wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=4153, passed=69351
Got 69351 stars (including 65059 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat
util/solve_plate_with_UCAC5 got 69351 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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits -region wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.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.zq7UhLYAH8 (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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=2739, passed=50772
Got 50772 stars (including 47969 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 50772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 969 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits -region wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.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.zh2ZDuwQ4f (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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2844, passed=50170
Got 50170 stars (including 47269 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 50170 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 968 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits -region wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/wcs_Tau-02-Q2b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits
Saving fully-calibrated image wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/wcs_Tau-02-Q2b1x1_2025-12-23_00-09-03_20.00sec_-14.90C_LIGHT_0289.fits
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-46-37_20.00sec_-14.90C_LIGHT_0058.fits
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.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_Tau-02-Q2b1x1_221342_TTUQ2b1x1_18616_d9ZQbVJ2/wcs_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059.fits
Preparing the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out84556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out01747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85282.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 32s
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: 12s
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Considering the candidate 84556_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84556_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:15:33.23 +26:22:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.521 118290790972184960 048.88799236536 +26.37164775459 13.7116 13.0762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84559_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84559_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:09:35.00 +24:40:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 3.637 111661697930323584 047.39692039508 +24.68210110049 13.5487 12.9361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84560_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84560_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:51:33.57 +17:51:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.859 43886250708681600 057.89012200984 +17.85909565745 13.8941 13.1672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84561_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84561_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:14:35.51 +26:13:07.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)
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Considering the candidate 84570_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84570_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:34:17.27 +24:32:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 2.459 68487587158252800 053.57204700769 +24.53309961844 14.3605 13.7350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84572_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84572_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:09:18.50 +24:44:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.609 111665271343000960 047.32726689250 +24.73755641276 13.3899 12.9111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84573_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84573_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:11:38.33 +25:10:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.468 112057728275380864 047.91043594858 +25.17147578853 13.2847 12.6598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84574_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84574_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:09:48.18 +26:40:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 4.301 112546495552484096 047.44945240220 +26.67509339671 13.2740 12.6804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84577_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84577_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 84584_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84584_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:14:35.83 +26:01:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.584 112228358734977408 048.65039411444 +26.02143213513 13.2821 12.6406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84585_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84585_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:10:08.58 +24:45:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.433 111668913475448576 047.53618162519 +24.75395838133 13.2148 12.6664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84591_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84591_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:14:27.58 +25:44:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.577 112196575976942336 048.61413323767 +25.73987991383 13.2445 12.6489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84595_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84595_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:28:23.91 +17:03:24.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 84596_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84596_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:08:55.90 +24:50:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.456 111720281284118400 047.23428048670 +24.84106918985 13.0932 12.5248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84597_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84597_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:35:06.09 +17:40:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 0.878 56357912320390784 053.77562958768 +17.67039205343 13.9489 13.3764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84598_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84598_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84600_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84600_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:09:21.62 +24:35:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.095 111660151742110592 047.33978276902 +24.58585556621 13.1170 12.3731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84602_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84602_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:30:46.23 +17:48:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.622 56584274276970496 052.69307389944 +17.80596880861 14.0838 13.5279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84604_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84604_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:10:16.55 +17:38:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.350 58633935748059904 047.56946835529 +17.64893577941 13.2611 12.7234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84605_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84605_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 84606_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84606_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:30:16.34 +20:47:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.711 58351292541521152 052.56852660814 +20.78626073392 13.5199 12.9146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84610_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84610_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:08:30.51 +23:45:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.361 110753398244997504 047.12671204701 +23.75624429140 13.0113 12.4435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84611_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84611_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 84618_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84618_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 04:13:14.20 +26:35:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.768 162750883672410624 063.30849890821 +26.58968226606 13.6336 13.2394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84619_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84619_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:11:26.03 +24:31:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.161 110899594635875328 047.85749334249 +24.52627452995 12.9410 12.2108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84622_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84622_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:58:48.02 +20:01:36.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 84629_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84629_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84633_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84633_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 84638_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84638_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:09:41.50 +23:31:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.997 110688935079841408 047.42187288990 +23.52977046045 12.6534 12.0713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84643_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84643_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84646_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84646_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 84647_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84647_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:08:59.32 +24:17:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.586 111618778319783424 047.24824071256 +24.29946274103 12.2635 11.5562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84650_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84650_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:45:47.03 +18:55:51.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
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Considering the candidate 84652_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84652_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 84654_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84654_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84656_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84656_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:10:01.04 +26:11:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.629 112377338263767168 047.50317352592 +26.18778290871 11.8042 11.2061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84662_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84662_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84663_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84663_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84673_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84673_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:45:09.75 +24:29:03.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 84677_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84677_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 84685_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84685_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 84687_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84687_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84691_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84691_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84692_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84692_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:20:23.14 +24:32:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84697_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84697_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84698_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84698_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 84699_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84699_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84700_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84700_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84705_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84705_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84709_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84709_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 84711_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84711_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84714_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84714_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 84715_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84715_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 84716_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84716_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 84717_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84717_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84718_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84718_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84719_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84719_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84722_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84722_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 84723_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84723_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84725_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84725_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84727_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84727_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 04:13:07.35 +26:40:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84729_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84729_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 84734_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84734_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 84735_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84735_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84736_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84736_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 84737_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84737_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 84738_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84738_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84739_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84739_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84741_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84741_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84744_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84744_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84745_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84745_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84746_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84746_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84749_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84749_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84750_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84750_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84751_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84751_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 84752_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84752_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 84754_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84754_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 84756_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84756_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 84757_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84757_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84759_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84759_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84760_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84760_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 84763_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84763_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84765_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84765_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84766_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84766_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84767_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84767_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84768_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84768_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:08:33.34 +26:55:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.813 115559844607307776 047.14071238360 +26.91656968611 12.2166 11.5629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84769_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84769_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:39:54.70 +25:11:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84770_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84770_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 84772_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84772_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 84773_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84773_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84774_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84774_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84776_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84776_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 84777_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84777_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 84778_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84778_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 84779_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84779_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 84780_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84780_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84783_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84783_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84784_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84784_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 84785_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84785_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 84789_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84789_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84790_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84790_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84791_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84791_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 84792_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84792_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 84794_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84794_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 84795_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84795_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:27:02.55 +24:51:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84796_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84796_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84797_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84797_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84798_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84798_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 84799_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84799_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84801_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84801_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84802_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84802_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 84803_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84803_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:46:15.27 +23:59:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84806_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84806_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 84809_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84809_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84812_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84812_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84813_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84813_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84814_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84814_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 84818_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84818_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84819_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84819_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84820_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84820_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 84823_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84823_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:31:22.86 +26:10:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84824_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84824_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84825_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84825_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:24:28.65 +22:02:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84826_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84826_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 84827_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84827_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 84829_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84829_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 84831_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84831_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 04:00:44.51 +20:24:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84832_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84832_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84833_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84833_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84835_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84835_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84836_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84836_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 84837_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84837_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84838_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84838_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 84839_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84839_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 84841_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84841_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 84842_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84842_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84844_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84844_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84845_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84845_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84846_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84846_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84852_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84852_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 84853_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84853_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84855_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84855_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84856_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84856_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84857_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84857_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84858_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84858_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 84859_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84859_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84860_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84860_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:10:44.76 +21:52:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.205 60795713047597824 047.68743863506 +21.87624936916 13.2779 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84862_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84862_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 84863_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84863_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84864_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84864_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:48:12.46 +26:35:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84865_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84865_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 84867_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84867_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84868_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84868_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84870_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84870_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84871_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84871_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:44:11.38 +25:53:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84873_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84873_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 84876_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84876_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 84877_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84877_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84878_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84878_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:33:55.26 +24:15:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84879_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84879_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84884_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84884_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 84886_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84886_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:51:23.41 +24:31:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84888_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84888_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84890_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84890_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84891_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84891_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 84892_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84892_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 84894_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84894_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 84896_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84896_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84897_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84897_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84899_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84899_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84904_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84904_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:45:19.71 +26:53:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84905_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84905_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84906_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84906_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84907_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84907_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 84908_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84908_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84909_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84909_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:18:15.28 +24:03:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.279 110964431462180736 049.56336076626 +24.06619700656 13.5409 12.7871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84910_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84910_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84912_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84912_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 84913_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84913_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 84915_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84915_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84916_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84916_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 84917_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84917_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84918_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84918_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84920_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84920_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 84922_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84922_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 84925_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84925_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 84926_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84926_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84927_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 84927_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 84928_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84928_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 84929_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84929_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:20:26.65 +25:41:14.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 84930_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84930_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 84931_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84931_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84932_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84932_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 04:02:00.60 +19:54:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.134 50552971962811648 060.50310902489 +19.90823606770 13.3297 12.5633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84937_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84937_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84938_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84938_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 84940_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84940_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84941_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84941_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84943_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84943_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 84944_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84944_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84945_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84945_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84947_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84947_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 84948_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84948_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:24:20.54 +24:45:09.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 84950_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84950_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 84951_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84951_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84952_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84952_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84953_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84953_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84954_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84954_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84955_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84955_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 84956_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84956_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 84957_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84957_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84959_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84959_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 84960_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84960_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 84961_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84961_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:49:02.07 +23:53:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84962_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84962_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84963_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84963_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 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 84964_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84964_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84965_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84965_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84966_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84966_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:15:43.68 +21:09:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.262 61995658190983296 048.93045219418 +21.15327097897 13.9046 13.0631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84967_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84967_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 84968_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84968_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:57:12.88 +25:15:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.054 67046402293363072 059.30391977219 +25.25803989485 13.7241 12.9687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84969_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84969_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 84970_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84970_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 84971_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84971_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 84974_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84974_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 84975_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84975_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 84976_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84976_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 04:08:23.57 +19:43:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.733 51801158177488896 062.09862368593 +19.72455252104 13.8206 13.2025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84977_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84977_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 84979_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84979_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84982_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84982_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 84983_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84983_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 84984_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84984_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 84987_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84987_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 84988_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84988_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 84990_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84990_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 84993_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84993_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 84994_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84994_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84995_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84995_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 84996_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84996_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 84997_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 84997_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 85000_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85000_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85003_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85003_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:21:12.28 +21:07:12.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 85004_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85004_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85005_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85005_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 85006_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85006_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 85007_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85007_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 85010_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85010_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 85011_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85011_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:24:45.72 +16:55:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 3.850 54970088126520704 051.19158601741 +16.92439272713 14.1866 13.6394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85012_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85012_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 85013_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85013_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 85015_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85015_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 85016_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85016_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85017_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85017_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 85018_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85018_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:51:14.86 +24:34:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.765 66658721365649792 057.81306646051 +24.58017610129 13.9488 13.3456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85019_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85019_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 85021_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85021_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 85022_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85022_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 85023_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85023_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 85026_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85026_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 85027_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85027_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 85028_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85028_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 85029_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85029_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 85031_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85031_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 85032_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85032_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85033_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85033_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 85034_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85034_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 85035_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85035_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 04:04:32.13 +26:03:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 2.474 162518165165692416 061.13439759213 +26.05433166176 14.1563 13.5411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85037_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85037_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 85041_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 85041_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 85042_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85042_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85043_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85043_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 85047_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85047_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:35:06.86 +26:34:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 3.116 69708800979738752 053.77919734729 +26.57121998689 14.1020 13.4357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85050_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85050_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 85051_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85051_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 85054_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85054_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 85059_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85059_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 85060_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85060_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 85063_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85063_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 85065_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85065_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85068_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85068_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 85069_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85069_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 85073_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85073_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85074_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85074_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 85076_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85076_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:50:37.68 +24:47:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.899 66852475931453696 057.65757713404 +24.78724351891 14.0957 13.4815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85077_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85077_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85079_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85079_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 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 85081_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85081_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:50:05.60 +26:02:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 4.302 69998075617588096 057.52465327724 +26.03693623920 14.2414 13.7029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85082_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85082_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 85083_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85083_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 85087_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85087_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85088_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85088_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 85089_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85089_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 85091_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85091_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85092_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85092_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 85093_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85093_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:45:47.05 +25:36:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.896 69923721143181184 056.44661369983 +25.60605071378 14.1930 13.5890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85095_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85095_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 85097_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85097_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85098_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85098_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85099_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85099_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 85100_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85100_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 85101_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85101_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85102_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85102_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 85104_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85104_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 85106_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85106_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 85108_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85108_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 85109_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85109_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85110_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85110_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 85111_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85111_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 85112_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85112_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 85114_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85114_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 85115_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85115_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:47:51.11 +23:26:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.834 64987394971433984 056.96290051614 +23.43485796424 14.4380 13.8396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85116_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85116_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 85117_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85117_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 85119_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85119_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 85120_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85120_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 85122_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85122_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:30:06.78 +24:33:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.829 68901140968978176 052.52772277878 +24.55336025742 14.2873 13.4542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85123_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85123_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85124_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85124_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85126_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85126_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 85127_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85127_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85128_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85128_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 85132_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85132_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85133_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85133_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 85134_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85134_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85135_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85135_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 85137_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85137_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 85139_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85139_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85140_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85140_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85142_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85142_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 85144_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85144_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 85149_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85149_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 85151_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85151_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 85156_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85156_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85158_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85158_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 85160_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85160_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 85162_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85162_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 85165_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85165_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:36:15.93 +25:00:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 3.726 68525657748391680 054.06692062023 +25.00499270527 14.6054 13.8893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85166_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85166_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85167_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85167_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 85170_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85170_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 85171_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85171_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85175_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85175_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 85176_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85176_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 85181_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85181_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 85183_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85183_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 85184_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85184_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 85185_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85185_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:30:58.75 +21:01:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 3.920 58379330087996032 052.74578512239 +21.02617948840 14.6176 13.9626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85186_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85186_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 85188_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85188_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 85191_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85191_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 85193_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85193_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 85195_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85195_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 85197_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85197_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 85198_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85198_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 85200_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85200_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 85201_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 85201_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 85202_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85202_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 85204_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85204_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 85207_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85207_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 85208_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85208_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 85213_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85213_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 85214_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85214_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 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 85215_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85215_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 85218_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85218_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 85227_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85227_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85231_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85231_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 85245_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85245_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 85249_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85249_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 85250_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85250_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 85252_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85252_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 85256_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85256_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 85259_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85259_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 85260_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85260_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 85266_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85266_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 85276_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85276_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 85280_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85280_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 85282_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 85282_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 85287_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85287_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 85289_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85289_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 85349_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 85349_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 07911_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 07911_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:47:34.31 +26:16:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47494_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 47494_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 04:05:41.99 +16:55:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25555_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 25555_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 01747_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 01747_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 37388_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 37388_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 04:11:22.65 +22:01:00.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 34696_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 34696_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 47535_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 47535_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 04853_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
Preparing report for the candidate 04853_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
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Considering the candidate 61929_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 61929_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks
**** FOUND 03:36:48.29 +19:41:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60795_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059
The candidate 60795_fd_Tau-02-Q2b1x1_2026-03-19_21-47-23_20.00sec_-14.90C_LIGHT_0059 did not pass the final checks