This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C
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 20.0977* 05 09 43.54 +20 31 07.4 11.3 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,2461119.5977,11.32,0.05,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 20260320.0977 11.32CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:09:43.54 +20:31:07.4 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 44 33.57 +23 21 04.1 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,2461119.5977,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.0977 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:33.57 +23:21:04.1 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 04 51.16 +25 41 33.0 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,2461119.5977,12.37,0.05,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 20260320.0977 12.37CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:51.16 +25:41:33.0 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 12.29 05:54:51.87 +17:22:22.6
191.02932 -4.09410 galactic Ori Second-epoch detections are separated by 1.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:54:51.87 +17:22:22.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0977* 05 54 51.87 +17 22 22.6 12.3 U Ori 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,2461119.5977,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0977 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:51.87 +17:22:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 10.72 05:03:57.31 +17:52:13.8
184.00136 -14.05903 galactic Tau Second-epoch detections are separated by 0.6" and 8.0 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 3407092969170074752 | 05:03:57.05 +17:52:13.6 (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 20.0977* 05 03 57.31 +17 52 13.8 10.7 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
Gaia DR3 3407092969170074752,2461119.5977,10.72,0.05,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 3407092969170074752 20260320.0977 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:57.31 +17:52:13.8 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 11 53.80 +19 04 09.8 14.5 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,2461119.5977,14.46,0.05,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 20260320.0977 14.46CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:53.80 +19:04:09.8 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 04 59 42.95 +26 31 04.6 14.4 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
Gaia DR3 153727775857085184,2461119.5977,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 153727775857085184 20260320.0977 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:42.95 +26:31:04.6 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 04 59 22.96 +25 15 46.6 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
target,2461119.5977,14.27,0.05,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 20260320.0977 14.27CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:22.96 +25:15:46.6 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 13.90 04:58:37.42 +26:52:47.2
175.82696 -9.73025 galactic Tau Second-epoch detections are separated by 0.3" and 7.7 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 | ATO J074.6548+26.8846 | 04:58:37.42 +26:52:47.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0977* 04 58 37.42 +26 52 47.2 13.9 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
ATO J074.6548+26.8846,2461119.5977,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.6548+26.8846 20260320.0977 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:37.42 +26:52:47.2 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 02 10.77 +26 42 01.1 14.2 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,2461119.5977,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0977 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:10.77 +26:42:01.1 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 14.03 04:59:51.71 +25:12:12.4
177.35596 -10.51884 galactic Tau Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:51.71 +25:12:12.4 (user input) | T | P | (position from user input) SpType: A5V (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 20.0977* 04 59 51.71 +25 12 12.4 14.0 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,2461119.5977,14.03,0.05,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 20260320.0977 14.03CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:51.71 +25:12:12.4 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 13.64 05:02:39.61 +26:48:34.1
176.43302 -9.05342 galactic Tau Second-epoch detections are separated by 5.2" and 7.0 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 | ATO J075.6671+26.8094 | 05:02:39.61 +26:48:34.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0977* 05 02 39.61 +26 48 34.1 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
ATO J075.6671+26.8094,2461119.5977,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J075.6671+26.8094 20260320.0977 13.64CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:39.61 +26:48:34.1 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 04 58 46.12 +26 38 07.4 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
target,2461119.5977,13.53,0.05,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 20260320.0977 13.53CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:46.12 +26:38:07.4 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 05 17.24 +26 51 19.6 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
target,2461119.5977,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0977 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:17.24 +26:51:19.6 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 04 59 14.35 +25 49 57.8 13.4 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
target,2461119.5977,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0977 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:14.35 +25:49:57.8 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 13.12 04:58:45.77 +26:08:03.1
176.44892 -10.15634 galactic Tau Second-epoch detections are separated by 7.0" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 153694206392758656 | 04:58:45.32 +26:08:05.3 (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 20.0977* 04 58 45.77 +26 08 03.1 13.1 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
Gaia DR3 153694206392758656,2461119.5977,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 153694206392758656 20260320.0977 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:45.77 +26:08:03.1 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 38 24.19 +22 40 45.0 13.2 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
Gaia DR3 3404214855751537408,2461119.5977,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3404214855751537408 20260320.0977 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:24.19 +22:40:45.0 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 13.13 05:00:51.35 +25:14:43.0
177.45883 -10.31378 galactic Tau Second-epoch detections are separated by 0.5" and 7.4 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 3419639320259790720 | 05:00:51.89 +25:14:44.6 (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 20.0977* 05 00 51.35 +25 14 43.0 13.1 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
Gaia DR3 3419639320259790720,2461119.5977,13.13,0.05,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 3419639320259790720 20260320.0977 13.13CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:51.35 +25:14:43.0 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 13.10 05:02:32.16 +26:43:58.1
176.47847 -9.12148 galactic Tau Second-epoch detections are separated by 2.0" and 7.4 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 | Large-amplitude variable Gaia DR2 3420442483439171968 | 05:02:32.72 +26:44:00.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
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 20.0977* 05 02 32.16 +26 43 58.1 13.1 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
Large-amplitude variable Gaia DR2 3420442483439171968,2461119.5977,13.10,0.05,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
Large-amplitude variable Gaia DR2 3420442483439171968 20260320.0977 13.10CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:32.16 +26:43:58.1 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 05 21.88 +18 08 26.7 12.6 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,2461119.5977,12.61,0.05,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 20260320.0977 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:21.88 +18:08:26.7 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 02 53.28 +21 56 18.9 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
VARIABLE_NAME,2461119.5977,12.81,0.05,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
VARIABLE_NAME 20260320.0977 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:53.28 +21:56:18.9 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 20 19.03 +18 14 23.9 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
VARIABLE_NAME,2461119.5977,12.81,0.05,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
VARIABLE_NAME 20260320.0977 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:19.03 +18:14:23.9 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 14 46.16 +19 06 03.4 13.4 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,2461119.5977,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.0977 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:46.16 +19:06:03.4 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 13.48 06:05:31.21 +26:11:52.7
184.58825 2.42881 galactic Gem Second-epoch detections are separated by 2.4" and 8.2 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 | Gaia DR3 3430061904517305344 | 06:05:32.24 +26:11:15.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0III 1967AJ.....72.1199M [M67b] +26 261
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3430061904517305344,2461119.5977,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3430061904517305344 20260320.0977 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:31.21 +26:11:52.7 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 12 16.35 +23 34 00.9 13.8 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,2461119.5977,13.82,0.05,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 20260320.0977 13.82CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:16.35 +23:34:00.9 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 13.92 05:59:55.91 +22:05:32.8
187.53325 -0.70338 galactic Ori Second-epoch detections are separated by 4.7" and 9.2 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 | 05:59:55.91 +22:05:32.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0977* 05 59 55.91 +22 05 32.8 13.9 U Ori 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,2461119.5977,13.92,0.05,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
target 20260320.0977 13.92CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:55.91 +22:05:32.8 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 31 44.93 +21 05 15.2 14.0 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,2461119.5977,14.03,0.05,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 20260320.0977 14.03CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:44.93 +21:05:15.2 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 22 45.93 +26 37 23.9 13.9 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
NSVS 6914926,2461119.5977,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6914926 20260320.0977 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:45.93 +26:37:23.9 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DO Gem,2461119.5977,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DO Gem 20260320.0977 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:26.72 +23:51:16.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 09 07.82 +26 08 15.8 11.6 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
V1252 Tau,2461119.5977,11.62,0.05,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
V1252 Tau 20260320.0977 11.62CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:09:07.82 +26:08:15.8 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 15 47.56 +26 45 13.7 12.3 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
NSVS J0515475+264514,2461119.5977,12.28,0.05,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
NSVS J0515475+264514 20260320.0977 12.28CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:47.56 +26:45:13.7 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 37 26.59 +22 20 31.1 12.5 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
V1259 Tau,2461119.5977,12.50,0.05,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
V1259 Tau 20260320.0977 12.50CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:26.59 +22:20:31.1 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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 20.0977* 05 53 50.42 +21 45 08.5 12.8 U Ori 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
NSVS J0553506+214506,2461119.5977,12.82,0.05,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
NSVS J0553506+214506 20260320.0977 12.82CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:50.42 +21:45:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 12.61 05:01:51.69 +17:21:33.1
184.13664 -14.76127 galactic Tau Second-epoch detections are separated by 0.3" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3405546948445590656 | 05:01:51.64 +17:21:33.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-0.026 (G)
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 20.0977* 05 01 51.69 +17 21 33.1 12.6 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
Gaia DR3 3405546948445590656,2461119.5977,12.61,0.05,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 3405546948445590656 20260320.0977 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:51.69 +17:21:33.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 11.27 05:02:06.34 +17:18:12.1
184.21855 -14.74581 galactic Tau Second-epoch detections are separated by 1.5" and 8.1 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 3405543344969504896 | 05:02:06.12 +17:18:09.4 (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 20.0977* 05 02 06.34 +17 18 12.1 11.3 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
Gaia DR3 3405543344969504896,2461119.5977,11.27,0.05,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 3405543344969504896 20260320.0977 11.27CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:06.34 +17:18:12.1 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0977 2461119.5977 13.02 06:05:42.26 +25:44:18.2
185.00999 2.24078 galactic Gem Second-epoch detections are separated by 1.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:05:42.26 +25:44:18.2 (user input) | T | P | (position from user input) J-Ks=0.291+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.5977,13.02,0.05,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 20260320.0977 13.02CV 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:42.26 +25:44:18.2 ;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-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20_00sec_-14_90C_LIGHT_0030_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: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461119.59958326 20.03.2026 02:23:13.994 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 22895
Objects passed selection criteria: 22883
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 21975.5
Average stars matched: 21408 (97.4176 %)
Memory usage VmPeak: 126084 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 21:41:00 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: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461119.59958326 20.03.2026 02:23:13.994 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 522
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 94 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): 162828
Objects passed selection criteria: 162439
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: 153510
Average stars matched: 148192 (96.5353 %)
Memory usage VmPeak: 2111832 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 21:44:21 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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: 2461119.59585390
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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits'
wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:18.264 +21:59:44.71
Angular distance between the image centers 0.01 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 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:21.664 +21:59:40.18
Angular distance between the image centers 0.01 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 05:32:18.264 +21:59:44.71
Second-epoch second image center 05:32:21.664 +21:59:40.18
Angular distance between the image centers 0.01320 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.IeoF4R1944
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.3j5gviTKPW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits &> /tmp/tmp.kMhB3OAp4F
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits &> /tmp/tmp.AF1jOsCuJp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat) found
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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 10157 out of 22997 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.956266
a=0.000000 b=1.000000 c=22.956266
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
2.0 pix Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
2.4 pix fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
2.4 pix fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.3 mag. Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
15.1 mag. fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
15.1 mag. fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (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.IeoF4R1944 (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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2479, passed=22997
Got 22997 stars (including 20487 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
util/solve_plate_with_UCAC5 got 22997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 936 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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.3j5gviTKPW (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-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2545, passed=22806
Got 22806 stars (including 20234 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 22806 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 934.0'
Seting catalog search parameters based on the expected field of view 934.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012972 (46.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010378 (37.4 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 616 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: 2.04"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 661 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.45"
Estimated accuracy of the plate solution: 1.58"
Excluding outliers - 624 stars left (next iteration limit 630)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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.kMhB3OAp4F (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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1828, passed=21871
Got 21871 stars (including 20027 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 21871 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AF1jOsCuJp (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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1869, passed=20768
Got 20768 stars (including 18874 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 20768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 931 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits'
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31489.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 31431_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31431_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:33:56.59 +21:19:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 3.116 3403641121135845760 083.48665716295 +21.31885213772 12.5125 12.1538 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 31433_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31433_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:20:00.66 +17:03:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.062 3394358249401659520 080.00281854262 +17.05190694052 12.3592 11.5421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31434_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31434_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:46:18.70 +18:27:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.856 3398366141084468736 086.57825533066 +18.45698556090 11.8030 10.8345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31436_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31436_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:07:18.89 +17:57:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.247 3407129695433560832 076.82876096557 +17.95182460670 11.9298 11.3607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31437_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31437_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:06:08.63 +25:14:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 0.429 3426592979686123008 091.53600958008 +25.24275136508 11.4312 10.9205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31440_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31440_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:56.76 +26:36:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 2.380 3430112516411176448 091.48579080283 +26.60881258937 10.4031 9.7776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31442_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 31442_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 31444_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 31444_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 31446_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31446_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:30:07.88 +21:23:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 2.698 3403687227607443968 082.53363531963 +21.39149112085 10.3615 8.9728 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31447_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31447_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:50:30.67 +22:39:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.184 3427288210337327616 087.62784690227 +22.65419447674 12.0023 11.6882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31448_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31448_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:15:47.56 +26:45:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 1.516 3420967397162562176 078.94783052894 +26.75421209315 11.0800 9.6633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31449_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31449_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:30:44.11 +20:13:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.162 3401302215087738624 082.68398545729 +20.23312788265 11.9649 11.4175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31450_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31450_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:47:52.51 +23:25:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.299 3427572919426796928 086.96878413057 +23.42044374847 12.0268 11.5697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31451_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31451_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:31:17.60 +21:32:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.637 3403706782596246912 082.82377309826 +21.53896786497 12.1081 11.5791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31452_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31452_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:32:49.60 +26:44:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.891 3441942333810826624 083.20725353357 +26.73788304883 12.1405 11.5142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31455_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31455_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:47:46.33 +23:58:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.482 3427746019490856448 086.94318636400 +23.98177106201 12.0917 11.7115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31456_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31456_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:43:24.71 +26:13:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.168 3441326572939651200 085.85324271628 +26.23242249087 11.9198 11.1069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31457_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31457_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:49:23.97 +21:18:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.748 3400131033343301888 087.34976175205 +21.30195666115 12.2720 11.8051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31463_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31463_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:55:16.39 +20:22:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.805 3399067973101282944 088.81852604008 +20.38287562051 12.4134 11.8903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31464_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31464_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:45:01.00 +26:19:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.059 3429339005682397952 086.25449321186 +26.32038629404 12.1180 11.5792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31467_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31467_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:30:53.96 +21:37:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.329 3403720045454648960 082.72577334394 +21.63216983911 11.6240 10.5460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31468_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31468_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:27:23.99 +22:56:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.228 3416050067629411840 081.85032830326 +22.93359708689 12.1026 11.4858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31469_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 31469_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 31470_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31470_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:31:11.79 +22:43:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.612 3404103809371717760 082.79930023921 +22.72405280964 12.0639 11.3547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31479_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31479_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:54:24.00 +22:43:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.712 3424389798904314368 088.60051527136 +22.71748371748 11.9599 11.1057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31487_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31487_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:46:55.00 +22:19:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.297 3403290995400723584 086.72919910130 +22.33202142283 12.2146 11.8831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31489_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 31489_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 31491_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31491_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:30:35.49 +23:55:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.504 3416622054194043392 082.64802095330 +23.93012447998 11.7498 10.6641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31492_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31492_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:40:07.76 +21:25:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.686 3403315042920172544 085.03241616397 +21.42364653183 12.1896 11.7163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31495_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31495_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:34:39.40 +23:44:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.841 3404573502698643968 083.66442075200 +23.74897937932 12.2202 11.6990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31496_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31496_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:44:16.78 +24:27:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.620 3428581579608585344 086.07010598713 +24.45805508665 11.9457 11.0024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31500_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31500_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:41:21.14 +22:49:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.360 3403557107277261184 085.33798136118 +22.83214496269 12.2692 11.7853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31503_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 31503_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:54:47.62 +21:47:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.609 3423984040457797632 088.69859382854 +21.78798385233 12.0018 11.2350 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 14186_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 14186_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:55:48.73 +20:10:33.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20535_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 20535_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 20s
Prepared the HTML report for the field Tau-04-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 ####
05:03:57.31 +17:52:13.8
05:09:43.54 +20:31:07.4
05:44:33.57 +23:21:04.1
05:04:51.16 +25:41:33.0
05:54:51.87 +17:22:22.6
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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:18.264 +21:59:44.71
Angular distance between the image centers 0.01 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 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:21.664 +21:59:40.18
Angular distance between the image centers 0.01 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 05:32:18.264 +21:59:44.71
Second-epoch second image center 05:32:21.664 +21:59:40.18
Angular distance between the image centers 0.01320 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.ko1zxMUOak
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.pVwptq39zB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits &> /tmp/tmp.U3pw2e8wf1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits &> /tmp/tmp.4P9WrbaPdK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat) found
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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 10499 out of 167968 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.793970
a=0.000000 b=1.000000 c=22.793970
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 215 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
1.9 pix Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
2.3 pix fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
2.2 pix fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
Limiting magnitude estimates:
15.5 mag. Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.5 mag. Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
15.3 mag. fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
15.3 mag. fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
All-image limiting magnitude estimate: 15.3 (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.ko1zxMUOak (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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=21684, passed=167940
Got 167940 stars (including 145994 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
util/solve_plate_with_UCAC5 got 167940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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.pVwptq39zB (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-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=21854, passed=169419
Got 169419 stars (including 147299 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 169419 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 934.0'
Seting catalog search parameters based on the expected field of view 934.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012972 (46.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010378 (37.4 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 589 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: 2.15"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.75"
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 643 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.74"
Estimated accuracy of the plate solution: 1.56"
Excluding outliers - 601 stars left (next iteration limit 606)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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.U3pw2e8wf1 (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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=17015, passed=139043
Got 139043 stars (including 121860 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 139043 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 925 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4P9WrbaPdK (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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=17210, passed=141901
Got 141901 stars (including 124516 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 141901 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Tau-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-17-51_20.00sec_-14.90C_LIGHT_0030.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.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-04-Q2b1x1_213748_TTUQ2b1x1_24698_Vs7Ipi2C/wcs_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031.fits
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out161213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193971.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out193983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193996.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194012.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194026.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194057.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194071.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194087.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194301.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194316.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194343.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194384.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194421.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194477.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194552.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194603.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194650.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194726.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194750.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194762.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out194774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out194753.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out07287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82933.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 59s
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: 21s
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Considering the candidate 193800_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193800_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:04:03.34 +18:46:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 2.873 3407452573895871616 076.01432647383 +18.77347504678 14.2299 13.4417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193805_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193805_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:38:21.04 +23:43:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.393 3404596837257375104 084.58797719527 +23.72106802312 14.2869 13.7095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193822_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193822_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:53:41.42 +17:55:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.866 3350104285072033536 088.42275656189 +17.92464733339 14.6137 14.0982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193824_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193824_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:45.14 +24:26:18.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)
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Considering the candidate 193827_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193827_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:59:06.70 +16:56:59.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 193837_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193837_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:46:18.81 +19:41:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.589 3399342477346885888 086.57877892916 +19.69597723667 14.4867 13.8507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193847_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193847_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:54.76 +18:55:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 5.776 3408162789687218688 074.97977526465 +18.92825915958 13.9328 13.3464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193854_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193854_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:57:58.46 +18:30:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.345 3350514570409725696 089.49397637310 +18.50891752188 14.2214 13.5661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193859_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193859_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 193860_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 193860_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 193864_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193864_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:42:26.98 +18:46:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.157 3399172671521027072 085.61250750013 +18.78075958022 14.2286 13.6333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193865_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193865_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:58.60 +17:47:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.581 3395079151072806656 077.74447961457 +17.79268120341 14.6228 13.9779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193873_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193873_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:38:15.16 +17:31:25.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)
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Considering the candidate 193874_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 193874_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 193876_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193876_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:04:16.89 +20:25:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.280 3374873258385263104 091.07063089902 +20.43045687717 14.2649 13.3936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193884_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193884_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 193885_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 193885_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 193891_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193891_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:58:57.17 +24:24:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 4.691 3419479998448442752 074.73897548736 +24.40462764543 13.6292 12.8806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193892_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193892_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:00:39.68 +17:15:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 3.698 3405551178989909504 075.16442050434 +17.26598444585 13.5644 12.7879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193893_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193893_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:11:35.35 +17:58:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.770 3395457696606672896 077.89752268159 +17.97677319034 14.2425 13.6335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193894_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193894_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:58:49.58 +24:59:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 3.010 3419795730084531200 074.70566402758 +24.99001252569 13.3921 12.7159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193896_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193896_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:21.39 +16:58:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.584 3394820838855602304 077.58908034994 +16.97696196024 14.5400 13.8853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193897_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193897_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:00:17.29 +18:19:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.809 3407342214711680896 075.07308891838 +18.32675104720 13.6133 12.8670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193900_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193900_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:03:38.85 +24:28:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 4.425 3418791463652426752 075.91121271529 +24.47637689170 13.6696 12.9576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193901_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193901_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:33.98 +26:49:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 5.061 153835248822554240 075.39304178906 +26.82655180700 13.2907 12.6226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193909_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193909_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:19:44.37 +22:18:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 3.241 3414736224250799104 079.93573722131 +22.31005597788 14.3959 13.5386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193914_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193914_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:28:58.96 +17:35:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.866 3400264692724141440 082.24591217326 +17.59719465892 14.1282 13.4932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193922_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193922_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:08.97 +24:15:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.286 3419474981926697216 074.78712644931 +24.26572073976 13.6159 12.8878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193923_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193923_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:00:49.28 +19:27:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 3.201 3408321810852873344 075.20627204259 +19.46488739966 13.7408 13.1611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193925_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193925_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:22:09.60 +21:24:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.515 3414341430856616064 080.54073710055 +21.41154805682 14.3674 13.6586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193929_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193929_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:02:35.31 +26:16:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.413 3429758061350185600 090.64716571935 +26.27302967139 14.0742 13.6041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193937_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193937_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:58:56.24 +24:12:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 5.485 3419473195220353280 074.73269215965 +24.20821534123 13.4441 12.7759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193939_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193939_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:19:46.33 +23:32:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 3.417 3417124947622827648 079.94400470928 +23.53695704356 14.4978 13.7544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193949_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193949_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:34:46.02 +17:22:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.168 3397114488832147968 083.69196529038 +17.38133436849 14.1182 13.8168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193950_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193950_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:06:41.05 +26:17:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 3.136 3420182036623155584 076.67199504806 +26.29502954245 13.4028 12.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193954_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193954_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:46:47.56 +18:53:41.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)
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Considering the candidate 193955_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193955_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:54:13.21 +25:28:23.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)
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Considering the candidate 193960_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193960_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 193963_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193963_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:02:03.67 +22:15:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.278 3412250022302108672 075.51625392230 +22.26561617737 14.2099 13.5663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193965_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193965_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:09:51.48 +26:45:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.393 3421718191806195072 077.46537714139 +26.75983002842 13.3269 12.5011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193968_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193968_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:28.66 +24:16:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 2.819 3419428321401956992 074.87015850753 +24.27395060323 13.7483 13.2454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193971_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193971_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:06:29.35 +25:57:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 3.066 3420143862954071680 076.62165840590 +25.95079986988 13.5890 12.5935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193979_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193979_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:38.94 +23:55:02.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)
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Considering the candidate 193983_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193983_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:22:36.43 +17:29:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.954 3394492600275856128 080.65173190312 +17.49034221923 13.9204 13.1648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193984_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193984_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:00:45.31 +23:39:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.208 3418639902846247936 075.18883523934 +23.65166760091 13.3109 12.6065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193992_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193992_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 193993_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193993_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:16:23.10 +19:52:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.620 3413765355483639808 079.09667071225 +19.88157541682 13.9329 13.1694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193996_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193996_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:28.08 +26:56:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 3.288 153840230984616448 075.36799753414 +26.94865325262 13.2410 12.4129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193999_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 193999_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:03:33.02 +26:15:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.479 3429748303184420608 090.88744745373 +26.26072557609 13.9189 13.5620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194001_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194001_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:49.77 +26:19:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 2.274 3430081008531741056 091.45800461766 +26.33122802564 14.0391 13.4801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194004_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194004_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194005_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194005_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:03:53.52 +25:48:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 5.887 3420056726656803840 075.97475958898 +25.81268413694 13.2668 12.5237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194007_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194007_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:56.72 +22:53:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.752 3412527752066891008 074.98581862869 +22.88766810427 13.2842 12.5947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194012_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194012_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:02:56.87 +25:26:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 3.499 3429635465804484224 090.73641043491 +25.44233660451 13.9663 13.1754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194014_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194014_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:40:40.74 +20:36:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.520 3402640599912545536 085.16991160968 +20.61072757763 13.8352 13.3291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194022_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194022_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:59:40.17 +16:45:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.426 3348984977937782272 089.91727475286 +16.75188422538 13.8550 13.3997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194023_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194023_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:15.20 +22:09:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.778 3412281805060019072 074.81444273305 +22.15874100337 13.2425 12.5412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194026_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194026_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:01:41.66 +17:46:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.717 3350180907288137088 090.42356022377 +17.77480979050 13.8610 13.2387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194031_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194031_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 194033_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194033_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:21.85 +24:25:20.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)
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Considering the candidate 194036_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194036_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194043_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194043_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:45.54 +25:35:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.939 3420225570411194496 074.94093695738 +25.59458717744 13.1482 12.4974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194045_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194045_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:34:33.73 +19:32:01.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
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Considering the candidate 194049_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194049_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:57:16.35 +18:04:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.499 3350426712559325824 089.31849747991 +18.06775317239 13.7141 13.1878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194051_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194051_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:02:34.48 +26:35:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 5.488 3420427979334953472 075.64197980756 +26.60016564988 13.3783 12.6129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194057_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194057_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:03:12.73 +26:00:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.659 3420253573597980416 075.80478035155 +26.00192083373 13.1671 12.5431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194065_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194065_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194068_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194068_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:39:43.99 +20:57:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.657 3402733641787274880 084.93363748046 +20.95182787006 13.5922 12.7276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194069_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194069_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:02:56.40 +26:23:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 5.462 3420369292901831936 075.73669366808 +26.38649580655 12.8162 12.0463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194071_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194071_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:55.73 +24:56:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.097 3419615788134578432 075.48265928569 +24.93625681804 13.1489 12.4202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194073_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194073_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:26:46.25 +18:01:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.255 3400352413135742592 081.69305234702 +18.02581524067 13.6211 13.0089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194087_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194087_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:04:24.81 +26:40:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.128 3430151480354614144 091.10246967817 +26.68170595261 14.0381 13.6564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194089_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194089_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194091_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194091_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:35:40.98 +20:49:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.337 3402811092935584512 083.92077434653 +20.82817625390 14.2980 13.6925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194096_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194096_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194099_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194099_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:52:15.30 +23:56:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.727 3427892293195778816 088.06343527502 +23.93555058925 13.6894 13.2303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194103_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194103_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:36:51.31 +24:44:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 0.883 3416736373340644096 084.21396640768 +24.73918708432 13.4311 12.8443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194105_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194105_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:22:08.86 +17:40:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.375 3394510089382664960 080.53701037517 +17.68102613076 13.6900 13.4326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194112_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194112_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:03:23.60 +24:58:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.499 3426514639485994240 090.84847137772 +24.97825401511 13.4709 13.1002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194113_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194113_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:58:58.57 +24:59:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.805 3419795794507627264 074.74380249178 +24.99730446837 12.6492 11.9665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194119_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194119_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 194120_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194120_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:19:06.17 +17:57:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.231 3395328332191763840 079.77602648943 +17.96510368808 13.2238 12.5758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194126_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194126_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194130_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194130_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194135_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194135_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:03:28.45 +26:16:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.625 3420363795343696896 075.86950101190 +26.26924549566 12.4462 11.5798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194136_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194136_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:39.42 +26:27:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.964 3420431179085869696 075.41441904979 +26.46267049216 12.3384 11.5476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194137_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194137_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 194147_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194147_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:38.65 +24:10:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.195 3419426431617224832 074.91105517135 +24.18283600577 13.1029 12.4930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194149_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194149_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:46:26.64 +25:17:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.140 3429021388558853888 086.61145246356 +25.28523664614 13.2158 12.5351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194151_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194151_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194153_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194153_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:46.83 +24:01:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.182 3419420178144508032 074.94359474822 +24.02617710567 12.7383 11.8811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194156_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194156_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194158_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194158_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194161_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194161_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:42:58.70 +20:06:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.154 3399596155295072512 085.74406095287 +20.10123156967 13.2135 12.8188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194162_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194162_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 194164_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194164_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:01:40.52 +26:42:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.397 3429975691634124800 090.41895667256 +26.70038933253 13.0481 12.6099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194167_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194167_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194169_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194169_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:00:57.88 +26:57:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.552 153852501708124672 075.24185782270 +26.96643439107 12.0930 11.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194171_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194171_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:34:30.71 +19:49:40.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 194179_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194179_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:21.38 +26:16:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 3.756 3420322082620711424 075.34013068105 +26.27667697008 11.8996 11.2111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194182_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194182_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:20.59 +26:15:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 2.657 3420322013901234944 075.33632890803 +26.26430909974 11.8712 11.2205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194184_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194184_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:13:11.17 +18:38:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.665 3395648423217597312 078.29664925100 +18.63390420876 12.4261 11.8298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194193_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194193_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:57:19.55 +19:56:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 1.002 3398805155460681344 089.33171815620 +19.94216140320 11.9162 11.4853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194194_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194194_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:32.24 +25:15:34.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)
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Considering the candidate 194195_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194195_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:07:18.91 +17:57:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.480 3407129695433560832 076.82876096557 +17.95182460670 11.9298 11.3607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194199_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194199_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 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 194201_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194201_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:56.73 +26:36:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 1.900 3430112516411176448 091.48579080283 +26.60881258937 10.4031 9.7776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194202_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194202_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:36.64 +25:57:57.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 194205_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194205_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:24:16.89 +20:08:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.65, MAG_FAINT_SEARCH_LIMIT=11.63)GAIADR2_OUTPUT=# 1.104 3402001302620712320 081.07060566452 +20.14699485784 10.3722 9.4443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194207_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194207_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:09:43.58 +20:31:07.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 194210_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194210_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:44:33.62 +23:21:04.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 194220_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194220_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:58:01.77 +25:55:16.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194228_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194228_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:04:51.25 +25:41:32.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 194235_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194235_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194249_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194249_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194254_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194254_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:05:41.72 +23:02:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.028 3418398147728086400 076.42376771404 +23.04055419150 12.6924 12.1336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194259_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194259_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194261_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194261_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:43:34.63 +25:27:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.076 3428896112952248960 085.89444044940 +25.46490598959 12.6959 12.2009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194262_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194262_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:35.50 +25:11:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.854 3426569134032793984 091.39811039435 +25.19177106080 13.2051 12.9401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194271_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194271_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:04:02.20 +25:15:52.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
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Considering the candidate 194277_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194277_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:04:13.33 +25:24:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.998 3426634451894841216 091.05575533148 +25.41286573379 12.6805 11.9593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194278_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194278_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:05:46.14 +26:25:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.463 3420381254386240896 076.44134569079 +26.42968567991 12.4233 11.5339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194285_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194285_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:45:54.25 +26:05:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.602 3429317359047201792 086.47642223942 +26.10014590108 12.8235 12.2081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194300_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194300_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:07:24.35 +18:37:06.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194301_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194301_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:47.47 +25:09:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.670 3426569168392518016 091.44827073172 +25.16455383340 13.2755 12.5330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194306_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194306_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:32:02.93 +18:33:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.079 3400807606659771136 083.01218604634 +18.56616114258 12.8533 12.0230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194314_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194314_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:24:11.85 +18:29:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.767 3400615402573507840 081.04987634144 +18.48424292872 13.3847 12.7931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194316_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194316_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:15:48.26 +21:07:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.253 3414166952106003200 078.95141535247 +21.13326990731 13.0004 12.0348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194321_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194321_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:39:49.78 +26:46:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.630 3441600243959904640 084.95800092131 +26.76754427643 13.5354 13.1361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194323_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194323_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:48:27.11 +20:53:28.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194337_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194337_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:56.39 +25:09:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.072 3426565968637284736 091.48485196648 +25.15007929907 13.5067 12.7467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194343_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194343_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:31:01.11 +20:27:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.593 3401331489584018432 082.75474958008 +20.45289918550 13.3749 12.8496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194347_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194347_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:55:14.51 +20:28:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.537 3399072581602946304 088.81076770861 +20.47136463130 13.2461 12.7076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194356_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194356_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:58:09.29 +21:58:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.105 3424057608953782272 089.53920827610 +21.97177315547 13.3996 12.7636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194358_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194358_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:52:52.71 +17:05:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.619 3349897302008816640 088.22072584275 +17.08906751684 13.4389 12.7445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194361_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194361_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194363_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194363_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:49:44.88 +24:06:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.518 3427727877548987264 087.43718891006 +24.10455959222 13.8523 13.4559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194369_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194369_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:48.69 +25:09:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.037 3419259271489847424 077.70277129911 +25.15372472444 13.0095 12.1001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194384_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194384_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:43:36.66 +25:27:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.817 3428896216031460352 085.90295658527 +25.46430227928 13.5912 13.1025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194387_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194387_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194400_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194400_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:07.17 +24:21:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.642 3426243747308184832 091.28014977273 +24.36124239974 13.5512 13.0790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194401_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194401_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:39:27.34 +21:47:32.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194406_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194406_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:31:04.40 +20:26:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.816 3401331425162099072 082.76865674796 +20.44495897834 13.3911 12.4456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194410_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194410_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:56:13.20 +17:26:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.449 3350012750729673984 089.05540871551 +17.43493359343 13.3824 12.8421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194421_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194421_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:36:20.93 +24:22:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.166 3416719880666498048 084.08691634126 +24.36710153197 13.7809 13.1577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194423_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194423_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 194434_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194434_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:13:30.22 +19:22:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.923 3407718969243759616 078.37634528513 +19.37193228135 13.7231 12.8449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194436_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194436_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:05.41 +22:29:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.002 3415294192042397696 077.52250491162 +22.49763834471 13.6678 12.9294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194440_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194440_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:00:17.06 +25:10:26.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 194448_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194448_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194453_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194453_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:27:58.73 +21:26:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 3.464 3402379294102701824 081.99564882078 +21.44212864089 13.8873 13.2537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194460_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194460_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:53:58.53 +21:51:17.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 194461_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194461_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:50:02.21 +17:07:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.511 3349935853635026304 087.50854802997 +17.12639461150 14.6874 14.2503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194463_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194463_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:59:33.79 +22:06:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.896 3424053657584077824 089.89132934673 +22.10460388132 13.9186 13.3259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194464_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194464_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:17:26.58 +18:34:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.535 3395419316778696320 079.36106636976 +18.57394210123 13.7757 12.8951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194466_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194466_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:34:57.27 +25:53:26.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 194472_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194472_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:03:28.20 +26:15:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 3.707 3429748337544163200 090.86852602605 +26.26310119008 13.2407 12.2035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194476_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194476_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:08:52.78 +19:50:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.194 3407983023833103872 077.21997532743 +19.83547855076 13.8813 13.2566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194477_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194477_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:37:26.45 +22:27:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.431 3404186685061563136 084.36055498557 +22.45512409039 13.7497 13.0008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194480_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194480_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:22:00.59 +18:15:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.520 3400596362981548544 080.50285236217 +18.25644302836 13.9987 12.9506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194481_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194481_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:06:23.71 +25:50:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.807 3427046253360190976 091.59824577287 +25.84539711426 13.9031 13.5981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194491_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194491_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194492_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194492_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:22:01.68 +18:15:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.457 3400596367278631040 080.50796338324 +18.26423603044 14.1305 13.4052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194499_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194499_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:47:37.25 +23:37:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.076 3427684756077637760 086.90540625773 +23.63354330745 13.7970 13.2290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194508_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194508_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:59:48.46 +25:21:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 4.052 3429598082407964416 089.95244457329 +25.36309163388 13.5471 12.5355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194512_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194512_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:58:05.48 +24:37:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.241 3427999289421997312 089.52351767214 +24.62064616943 13.7976 13.1199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194514_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194514_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 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 194536_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194536_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:36:30.61 +25:57:49.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194537_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 194537_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 194543_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194543_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:03:15.94 +16:56:22.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 194544_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194544_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:57:10.32 +21:28:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 4.037 3424004007762263936 089.29407355508 +21.47406518082 13.1339 11.8792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194552_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194552_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:50:26.27 +23:40:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.680 3427509521413864320 087.61021130097 +23.67736349523 13.7877 12.8515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194573_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194573_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:53:00.85 +17:17:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.145 3350044838426044160 088.25370410931 +17.29538864343 13.9399 13.4262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194574_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194574_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:25:00.83 +18:19:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 2.166 3400564069124720000 081.25367654475 +18.32939808765 14.3380 13.7536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194579_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194579_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:42:50.65 +17:22:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.359 3396730209519094272 085.71138394690 +17.37264415607 13.9898 13.2886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194582_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194582_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:51:02.17 +24:55:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 4.455 3428210189494701696 087.75952271820 +24.92667535946 14.2486 13.7537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194585_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194585_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:15:53.84 +17:16:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 3.478 3395163680325355264 078.97530894730 +17.28268853865 14.3218 13.5779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194591_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194591_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:54:10.28 +24:05:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.816 3427912393642582144 088.54338804130 +24.08673504086 14.2607 13.7054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194592_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194592_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:32:25.48 +26:59:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 4.572 3441998061008594304 083.10510463723 +27.00026370374 14.3441 13.6954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194602_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194602_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:48:20.04 +25:31:31.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)
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Considering the candidate 194603_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194603_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:57:03.19 +23:53:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.868 3424845890071164416 089.26412915737 +23.89191923198 14.2931 13.7235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194604_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194604_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:17:33.58 +24:02:03.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)
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Considering the candidate 194626_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194626_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:59:42.53 +26:31:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.233 3429947761465196160 089.92723212392 +26.53208900003 14.0613 13.4996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194643_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194643_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:34:19.87 +20:16:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.649 3402757045067540352 083.58266585738 +20.28219844631 14.5206 13.8595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194650_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194650_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:32:21.23 +20:56:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 3.435 3403599442773379328 083.08940460540 +20.94749836953 14.4401 13.7405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194657_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194657_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:14:45.82 +19:44:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 5.217 3413748484852144128 078.69210618043 +19.74669782434 14.3188 13.3876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194665_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194665_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:47:58.62 +24:26:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.788 3428544028713747712 086.99461634332 +24.44896523027 14.2526 13.4217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194669_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194669_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:31:18.33 +19:54:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.872 3401228895702932736 082.82749139725 +19.91159536668 14.4304 13.8114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194674_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194674_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:02:36.83 +19:09:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 3.358 3374624150285665152 090.65415074958 +19.15160934237 14.0348 13.0113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194682_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194682_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:17:07.42 +17:38:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 2.037 3395202163232219392 079.28150703280 +17.63360721302 14.5185 13.8840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194691_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194691_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:37:19.60 +26:53:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.942 3441286092872200448 084.33219519558 +26.89726567942 13.8633 12.8095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194692_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194692_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:23:00.21 +19:32:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.909 3401570843818488960 080.75132002026 +19.54910228286 14.3970 13.7083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194697_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194697_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:11:49.66 +17:13:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 3.941 3394854614478567552 077.95781651740 +17.23115016633 14.7841 14.1433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194722_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194722_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:39:28.57 +21:47:27.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194726_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194726_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:41:48.20 +21:43:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.448 3403161493546046592 085.45097224187 +21.71868653221 14.2508 13.7021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194730_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194730_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:44:00.96 +18:08:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.296 3398336355489194752 086.00398799129 +18.15002636082 14.3602 13.8201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194746_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194746_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:33:33.61 +21:42:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.665 3403759490434551808 083.39029175554 +21.71645295999 14.2352 13.3212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194748_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194748_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:50:58.13 +20:22:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.681 3399814889390638336 087.74297747346 +20.37507570221 14.4135 13.8601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194750_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194750_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:20:18.51 +23:09:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.520 3414850912761193984 080.07682371042 +23.16142988782 13.8875 12.8221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194751_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194751_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:37:29.52 +20:46:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 2.808 3402891834025670400 084.37362728321 +20.76920883671 14.5088 13.9309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194753_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194753_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:32:41.24 +17:30:13.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 194762_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194762_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:58:55.52 +26:28:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.338 3429987653121082240 089.73070839116 +26.47278111666 14.3202 13.4309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194768_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194768_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:48.90 +26:17:45.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 194774_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 194774_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:45:20.34 +21:58:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 4.741 3403254196121204864 086.33504844119 +21.98414873042 14.3766 13.4007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179418_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 179418_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks
**** FOUND 06:05:56.66 +23:44:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.738 3426142076843518592 091.48539385371 +23.73984117270 12.0843 11.5944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 09435_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 09435_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 46902_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 46902_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 15261_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 15261_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 07287_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 07287_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 74248_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 74248_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 82933_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 82933_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 161456_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 161456_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 160173_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 160173_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 16763_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
Preparing report for the candidate 16763_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
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Considering the candidate 161213_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031
The candidate 161213_fd_Tau-04-Q2b1x1_2026-03-19_21-23-13_20.00sec_-15.00C_LIGHT_0031 did not pass the final checks