This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DT Aur,2461119.5908,10.94,0.05,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
DT Aur 20260320.0908 10.94CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:10:32.21 +32:10:43.0 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 26 30.52 +25 53 48.4 12.1 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
ASAS J042630+2553.7,2461119.5908,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J042630+2553.7 20260320.0908 12.14CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:30.52 +25:53:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3449524561701744000,2461119.5908,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3449524561701744000 20260320.0908 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:19.18 +34:10:42.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 05 04 50.97 +25 41 31.1 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
VARIABLE_NAME,2461119.5908,12.35,0.05,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 20260320.0908 12.35CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:50.97 +25:41:31.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 14.36 04:28:00.76 +33:37:09.0
166.27315 -10.46605 galactic Per Second-epoch detections are separated by 3.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:28:00.76 +33:37:09.0 (user input) | T | P | (position from user input) SpType: F0 (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 20.0908* 04 28 00.76 +33 37 09.0 14.4 U Per 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,2461119.5908,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:00.76 +33:37:09.0 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 14.29 04:26:39.38 +34:18:22.2
165.56734 -10.20350 galactic Per Second-epoch detections are separated by 2.2" and 5.1 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 | target | 04:26:39.38 +34:18:22.2 (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 20.0908* 04 26 39.38 +34 18 22.2 14.3 U Per 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,2461119.5908,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:39.38 +34:18:22.2 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 14.11 04:25:05.12 +30:49:29.1
167.93503 -12.82040 galactic Tau Second-epoch detections are separated by 1.9" and 5.2 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 | 04:25:05.12 +30:49:29.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 25 05.12 +30 49 29.1 14.1 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
target,2461119.5908,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:05.12 +30:49:29.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.90 04:25:44.17 +32:34:37.4
166.71961 -11.52492 galactic Per Second-epoch detections are separated by 2.3" and 5.3 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 | 04:25:44.17 +32:34:37.4 (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 20.0908* 04 25 44.17 +32 34 37.4 13.9 U Per 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,2461119.5908,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:44.17 +32:34:37.4 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 24 01.37 +32 28 44.5 14.0 U Per 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,2461119.5908,14.00,0.05,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 20260320.0908 14.00CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:01.37 +32:28:44.5 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 14.03 04:25:36.36 +34:14:49.5
165.46009 -10.40209 galactic Per Second-epoch detections are separated by 2.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:25:36.36 +34:14:49.5 (user input) | T | P | (position from user input) SpType: A6IV (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 20.0908* 04 25 36.36 +34 14 49.5 14.0 U Per 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,2461119.5908,14.03,0.05,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 20260320.0908 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:36.36 +34:14:49.5 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 14.15 04:25:20.39 +31:38:59.8
167.35394 -12.21864 galactic Per Second-epoch detections are separated by 2.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:25:20.39 +31:38:59.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 25 20.39 +31 38 59.8 14.2 U Per 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,2461119.5908,14.15,0.05,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 20260320.0908 14.15CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:20.39 +31:38:59.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 14.03 04:25:42.73 +33:05:28.2
166.33312 -11.17744 galactic Per Second-epoch detections are separated by 3.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:25:42.73 +33:05:28.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 25 42.73 +33 05 28.2 14.0 U Per 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,2461119.5908,14.03,0.05,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 20260320.0908 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:42.73 +33:05:28.2 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 25 32.58 +30 21 05.1 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
Gaia DR3 165378407223674880,2461119.5908,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 165378407223674880 20260320.0908 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:32.58 +30:21:05.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.89 04:25:34.61 +34:09:16.1
165.52442 -10.46999 galactic Per Second-epoch detections are separated by 1.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:25:34.61 +34:09:16.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 25 34.61 +34 09 16.1 13.9 U Per 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,2461119.5908,13.89,0.05,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 20260320.0908 13.89CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:34.61 +34:09:16.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 23 58.12 +32 46 56.8 13.9 U Per 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,2461119.5908,13.95,0.05,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 20260320.0908 13.95CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:58.12 +32:46:56.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 25 54.39 +34 07 07.1 13.8 U Per 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,2461119.5908,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:54.39 +34:07:07.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.83 04:26:58.85 +33:16:03.0
166.38634 -10.86307 galactic Per Second-epoch detections are separated by 2.7" and 5.1 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 | target | 04:26:58.85 +33:16:03.0 (user input) | T | P | (position from user input) SpType: F4 (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 20.0908* 04 26 58.85 +33 16 03.0 13.8 U Per 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,2461119.5908,13.83,0.05,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 20260320.0908 13.83CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:58.85 +33:16:03.0 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 24 00.59 +33 17 53.2 13.6 U Per 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 172716101151307008,2461119.5908,13.61,0.05,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 172716101151307008 20260320.0908 13.61CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:00.59 +33:17:53.2 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.82 04:25:07.37 +33:57:30.0
165.60397 -10.67296 galactic Per Second-epoch detections are separated by 2.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 172806776500639616 | 04:25:08.32 +33:58:14.9 (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 20.0908* 04 25 07.37 +33 57 30.0 13.8 U Per 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 172806776500639616,2461119.5908,13.82,0.05,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
Gaia DR3 172806776500639616 20260320.0908 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:07.37 +33:57:30.0 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 26 33.27 +34 20 32.3 13.8 U Per 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,2461119.5908,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:33.27 +34:20:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.79 04:28:07.70 +34:28:18.2
165.65483 -9.86853 galactic Per Second-epoch detections are separated by 1.3" and 5.1 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 | target | 04:28:07.70 +34:28:18.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 28 07.70 +34 28 18.2 13.8 U Per 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,2461119.5908,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:07.70 +34:28:18.2 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.81 04:24:53.81 +33:22:54.0
165.99835 -11.10281 galactic Per Second-epoch detections are separated by 1.7" and 4.6 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 | 04:24:53.81 +33:22:54.0 (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 20.0908* 04 24 53.81 +33 22 54.0 13.8 U Per 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,2461119.5908,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:53.81 +33:22:54.0 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.63 04:28:59.89 +34:49:15.1
165.51866 -9.49990 galactic Per Second-epoch detections are separated by 2.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:28:59.89 +34:49:15.1 (user input) | T | P | (position from user input) SpType: F0 (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 20.0908* 04 28 59.89 +34 49 15.1 13.6 U Per 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,2461119.5908,13.63,0.05,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 20260320.0908 13.63CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:59.89 +34:49:15.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.68 04:24:53.05 +33:24:42.2
165.97421 -11.08412 galactic Per Second-epoch detections are separated by 2.8" and 5.1 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 | target | 04:24:53.05 +33:24:42.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 24 53.05 +33 24 42.2 13.7 U Per 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,2461119.5908,13.68,0.05,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 20260320.0908 13.68CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:53.05 +33:24:42.2 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.72 04:28:08.59 +33:46:22.2
166.17730 -10.34170 galactic Per Second-epoch detections are separated by 2.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:28:08.59 +33:46:22.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 28 08.59 +33 46 22.2 13.7 U Per 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,2461119.5908,13.72,0.05,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
target 20260320.0908 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:08.59 +33:46:22.2 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.56 04:28:11.25 +34:11:28.7
165.87188 -10.05042 galactic Per Second-epoch detections are separated by 5.6" and 5.3 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 | 04:28:11.25 +34:11:28.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 28 11.25 +34 11 28.7 13.6 U Per 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,2461119.5908,13.56,0.05,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 20260320.0908 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:11.25 +34:11:28.7 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 24 11.27 +32 49 38.1 13.6 U Per 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 172591409660415616,2461119.5908,13.58,0.05,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 172591409660415616 20260320.0908 13.58CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:11.27 +32:49:38.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.57 04:25:49.16 +33:41:44.5
165.89950 -10.74764 galactic Per Second-epoch detections are separated by 3.9" and 5.3 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 | 04:25:49.16 +33:41:44.5 (user input) | T | P | (position from user input) SpType: F0 (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 20.0908* 04 25 49.16 +33 41 44.5 13.6 U Per 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,2461119.5908,13.57,0.05,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 20260320.0908 13.57CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:49.16 +33:41:44.5 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 24 38.61 +33 28 25.7 13.6 U Per 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,2461119.5908,13.59,0.05,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 20260320.0908 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:38.61 +33:28:25.7 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.52 04:24:00.75 +33:42:14.1
165.63077 -11.01531 galactic Per Second-epoch detections are separated by 3.1" and 4.4 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 | ATO J066.0065+33.7032 | 04:24:00.11 +33:42:15.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (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 20.0908* 04 24 00.75 +33 42 14.1 13.5 U Per 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 J066.0065+33.7032,2461119.5908,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J066.0065+33.7032 20260320.0908 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:00.75 +33:42:14.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.62 04:26:16.71 +34:31:04.8
165.35623 -10.11538 galactic Per Second-epoch detections are separated by 3.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:26:16.71 +34:31:04.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 26 16.71 +34 31 04.8 13.6 U Per 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,2461119.5908,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:16.71 +34:31:04.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 23 51.46 +32 37 16.0 13.4 U Per 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,2461119.5908,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.0908 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:51.46 +32:37:16.0 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.46 04:25:01.94 +34:20:42.9
165.30482 -10.42085 galactic Per Second-epoch detections are separated by 2.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J066.2663+34.3473 | 04:25:01.94 +34:20:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 25 01.94 +34 20 42.9 13.5 U Per 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 J066.2663+34.3473,2461119.5908,13.46,0.05,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
ATO J066.2663+34.3473 20260320.0908 13.46CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:01.94 +34:20:42.9 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 23 35.93 +34 29 20.8 13.5 U Per 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,2461119.5908,13.48,0.05,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 20260320.0908 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:35.93 +34:29:20.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.46 04:26:54.25 +32:49:03.7
166.71082 -11.18110 galactic Per Second-epoch detections are separated by 1.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 172486475019544960 | 04:26:54.84 +32:49:04.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (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 20.0908* 04 26 54.25 +32 49 03.7 13.5 U Per 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 172486475019544960,2461119.5908,13.46,0.05,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
Gaia DR3 172486475019544960 20260320.0908 13.46CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:54.25 +32:49:03.7 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.27 04:27:14.44 +34:37:45.8
165.41126 -9.89470 galactic Per Second-epoch detections are separated by 3.1" and 4.4 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 173239262527435904 | 04:27:13.95 +34:37:48.1 (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 20.0908* 04 27 14.44 +34 37 45.8 13.3 U Per 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 173239262527435904,2461119.5908,13.27,0.05,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 173239262527435904 20260320.0908 13.27CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:14.44 +34:37:45.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.47 04:27:03.57 +34:40:41.3
165.34929 -9.88860 galactic Per Second-epoch detections are separated by 3.2" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 173240357742712576 | 04:27:04.38 +34:40:41.2 (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 20.0908* 04 27 03.57 +34 40 41.3 13.5 U Per 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 173240357742712576,2461119.5908,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 173240357742712576 20260320.0908 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:03.57 +34:40:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.24 04:24:36.16 +34:21:29.7
165.23321 -10.47629 galactic Per Second-epoch detections are separated by 4.7" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 176205882338909568 | 04:24:35.52 +34:21:32.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (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 20.0908* 04 24 36.16 +34 21 29.7 13.2 U Per 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 176205882338909568,2461119.5908,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 176205882338909568 20260320.0908 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:36.16 +34:21:29.7 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 25 02.94 +34 52 58.8 13.3 U Per 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 176257765543588352,2461119.5908,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 176257765543588352 20260320.0908 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:02.94 +34:52:58.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 13.14 04:27:12.93 +33:58:44.5
165.89052 -10.34235 galactic Per Second-epoch detections are separated by 3.6" and 5.2 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 | CSS_J042715.1+335848 | 04:27:13.59 +33:58:45.6 (Gaia DR3) | RS (local) | 0.872112300000 (local) | Gaia3var=NOT_AVAILABLE SpType: F8 (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 20.0908* 04 27 12.93 +33 58 44.5 13.1 U Per 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
CSS_J042715.1+335848,2461119.5908,13.14,0.05,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
CSS_J042715.1+335848 20260320.0908 13.14CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:12.93 +33:58:44.5 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 12.97 04:26:26.58 +33:42:15.9
165.98329 -10.64702 galactic Per Second-epoch detections are separated by 1.5" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 173124775879553536 | 04:26:26.03 +33:42:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 26 26.58 +33 42 15.9 13.0 U Per 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 173124775879553536,2461119.5908,12.97,0.05,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 173124775879553536 20260320.0908 12.97CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:26.58 +33:42:15.9 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 12.93 04:24:24.79 +30:11:53.2
168.30539 -13.35285 galactic Tau Second-epoch detections are separated by 1.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 165373184543371776 | 04:24:24.21 +30:11:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 24 24.79 +30 11 53.2 12.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 165373184543371776,2461119.5908,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 165373184543371776 20260320.0908 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:24.79 +30:11:53.2 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 12.73 04:27:19.45 +33:41:49.8
166.11587 -10.51796 galactic Per Second-epoch detections are separated by 3.4" and 5.1 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 | ATO J066.8406+33.6992 | 04:27:20.08 +33:41:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 27 19.45 +33 41 49.8 12.7 U Per 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 J066.8406+33.6992,2461119.5908,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J066.8406+33.6992 20260320.0908 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:19.45 +33:41:49.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 12.51 04:28:26.03 +34:28:50.8
165.69159 -9.81623 galactic Per Second-epoch detections are separated by 1.2" and 4.6 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 | ATO J067.1073+34.4904 | 04:28:26.64 +34:28:50.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 (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 20.0908* 04 28 26.03 +34 28 50.8 12.5 U Per 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 J067.1073+34.4904,2461119.5908,12.51,0.05,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 J067.1073+34.4904 20260320.0908 12.51CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:26.03 +34:28:50.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 12.29 04:25:58.95 +33:48:03.4
165.84502 -10.65088 galactic Per Second-epoch detections are separated by 3.5" and 5.1 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 172754068661986816 | 04:25:59.71 +33:48:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.0908* 04 25 58.95 +33 48 03.4 12.3 U Per 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 172754068661986816,2461119.5908,12.29,0.05,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
Gaia DR3 172754068661986816 20260320.0908 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:58.95 +33:48:03.4 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.5908,12.97,0.05,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 20260320.0908 12.97CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:46.35 +31:05:53.0 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 14.17 05:15:27.28 +30:39:39.4
174.95967 -4.51967 galactic Aur Second-epoch detections are separated by 3.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 180201404516175616 | 05:15:26.40 +30:39:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 180201404516175616,2461119.5908,14.17,0.05,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 180201404516175616 20260320.0908 14.17CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:27.28 +30:39:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.5908,14.19,0.05,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
VARIABLE_NAME 20260320.0908 14.19CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:28.19 +30:16:23.6 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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
BI Aur,2461119.5908,11.74,0.05,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
BI Aur 20260320.0908 11.74CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:37.50 +29:52:08.8 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 37 39.60 +32 37 26.1 10.5 U Per 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
V0657 Per,2461119.5908,10.50,0.05,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
V0657 Per 20260320.0908 10.50CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:39.60 +32:37:26.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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
V0482 Aur,2461119.5908,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0482 Aur 20260320.0908 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:10:41.79 +33:57:11.7 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.0908 2461119.5908 12.22 04:26:37.17 +27:10:15.1
170.94728 -15.03780 galactic Tau Second-epoch detections are separated by 0.8" and 5.1 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 152217012520954112 | 04:26:36.91 +27:10:14.1 (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 20.0908* 04 26 37.17 +27 10 15.1 12.2 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 152217012520954112,2461119.5908,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 152217012520954112 20260320.0908 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:37.17 +27:10:15.1 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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
NSVS J0513113+335055,2461119.5908,13.58,0.05,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 J0513113+335055 20260320.0908 13.58CV 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:11.24 +33:50:53.4 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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 20.0908* 04 23 21.08 +34 29 48.8 13.0 U Per 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 176222370716873984,2461119.5908,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 176222370716873984 20260320.0908 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:21.08 +34:29:48.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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
MY Aur,2461119.5908,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MY Aur 20260320.0908 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:21.32 +30:55:35.5 ;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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20_00sec_-14_90C_LIGHT_0022_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: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461119.59107925 20.03.2026 02:10:59.247 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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.: -7.59
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): 16019
Objects passed selection criteria: 16007
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 15448.5
Average stars matched: 15065.5 (97.5208 %)
Memory usage VmPeak: 120576 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 21:43:20 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: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461119.59107925 20.03.2026 02:10:59.247 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 477
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 78 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): 122225
Objects passed selection criteria: 121977
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: 114706
Average stars matched: 110681 (96.4912 %)
Memory usage VmPeak: 1902524 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 21:46:05 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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: 2461119.59052963
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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
Saving wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits to local_wcs_cache/
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
Saving wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits to local_wcs_cache/
'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits'
wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:00.197 +29:59:30.96
Angular distance between the image centers 0.00 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 05:00:01.017 +29:59:40.48
Second-epoch image center 04:59:57.984 +29:59:21.78
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 05:00:00.197 +29:59:30.96
Second-epoch second image center 04:59:57.984 +29:59:21.78
Angular distance between the image centers 0.00838 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.UZtjRLfDGR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.tiUd3JskvJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits &> /tmp/tmp.HwhMjo9s9I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.PwoRNzgCUg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
The reference image (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat) found
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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 6742 out of 16295 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.979657
a=0.000000 b=1.000000 c=22.979657
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 31 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.5 pix fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
2.5 pix fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
Limiting magnitude estimates:
15.4 mag. Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.4 mag. Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
15.1 mag. fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
15.1 mag. fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.UZtjRLfDGR (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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1498, passed=16295
Got 16295 stars (including 14768 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
util/solve_plate_with_UCAC5 got 16295 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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 955 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: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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.tiUd3JskvJ (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/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1486, passed=16349
Got 16349 stars (including 14839 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
util/solve_plate_with_UCAC5 got 16349 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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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.HwhMjo9s9I (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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1025, passed=14710
Got 14710 stars (including 13674 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 14710 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 953 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: 0.65"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PwoRNzgCUg (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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=999, passed=14852
Got 14852 stars (including 13840 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 14852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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 953 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: 0.63"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
Saving fully-calibrated image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits'
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out21135.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out21133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21150.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 21123_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21123_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 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 21126_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21126_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:05.54 +33:27:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 4.737 172766472527705728 066.02464097324 +33.46337457029 11.2890 10.7583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21128_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21128_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:35:46.77 +32:32:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 2.662 3448811773224818304 083.94569639233 +32.54953755780 10.9205 9.6706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21132_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21132_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:49:21.32 +30:55:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.91, MAG_FAINT_SEARCH_LIMIT=11.89)GAIADR2_OUTPUT=# 1.023 160165760035864832 072.33850287130 +30.92650981701 11.6351 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21133_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 21133_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 21134_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21134_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:36:07.72 +34:09:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 0.761 3449519304660746624 084.03226478408 +34.15694528894 11.5426 11.2970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21135_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21135_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:16:37.52 +29:52:08.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)
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Considering the candidate 21136_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21136_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:27:41.45 +34:26:43.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21138_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21138_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:10:41.82 +33:57:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 4.624 182185919925046400 077.67555095588 +33.95397430578 11.8203 9.9574 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21140_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 21140_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 21142_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 21142_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 21143_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21143_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:06:25.46 +34:49:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.789 184927208571518848 076.60632601308 +34.82501687114 12.2618 11.7355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21144_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21144_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:04:00.24 +33:52:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.199 184767672010076416 076.00132491829 +33.87952866308 11.9106 11.0417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21145_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21145_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:33:36.74 +33:40:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.309 3449117879836851840 083.40347245664 +33.66727653414 12.0417 11.5228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21147_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21147_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:02:11.57 +31:01:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.655 157356159932608512 075.54839340727 +31.02461703718 12.0817 11.4745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21148_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21148_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:36:41.46 +31:27:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.257 159688636411939328 069.17315345549 +31.45869859700 12.2285 11.5687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21150_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 21150_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 21152_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21152_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:06:18.07 +30:36:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.471 156358628008411776 076.57543968261 +30.60855797681 12.1661 11.6031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21153_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21153_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:20:52.08 +31:00:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.838 3446921708439316864 080.21724178407 +31.01635612392 12.1474 11.6277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21154_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21154_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:27:47.59 +32:38:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.058 3448987037951416960 081.94852808360 +32.64849384343 12.4321 12.2243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21155_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21155_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:11:54.26 +29:31:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.674 156084132357091200 077.97620341171 +29.52346083235 12.2420 11.5933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21156_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21156_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:38:19.69 +31:18:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 4.247 159630637173582464 069.58067559348 +31.31328347481 10.8707 9.5120 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21157_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21157_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:59:17.97 +30:58:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.890 156992049785449600 074.82512217818 +30.96945591751 11.9571 10.9850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21158_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21158_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:01:04.87 +29:17:47.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)
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Considering the candidate 21161_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21161_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:16:41.14 +33:09:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.047 181117293403579776 079.17176192117 +33.15736649406 11.8264 10.8204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21164_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21164_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:05:23.07 +32:31:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.808 181622415917709440 076.34639083476 +32.52098584918 11.9438 11.0428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21165_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21165_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:56:55.40 +29:03:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.259 156571216007157760 074.23117494152 +29.05662672354 12.2222 11.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21166_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21166_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:54:33.05 +29:45:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 0.835 156807469270576384 073.63797461052 +29.76279536052 12.2648 11.5784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21167_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21167_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:00:48.43 +30:38:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.920 156781360166717440 075.20208809208 +30.64626499638 12.3152 11.8435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21169_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21169_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:28:19.64 +34:16:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.311 182622597841683584 082.08186239613 +34.27661080857 12.4480 12.1240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21171_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 21171_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:21:48.20 +29:54:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.073 3446598726897186560 080.45117624820 +29.91084015796 12.0571 11.2308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Aur-05-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 ####
05:10:32.21 +32:10:43.0
04:26:30.52 +25:53:48.4
05:36:19.18 +34:10:42.1
05:04:50.97 +25:41:31.1
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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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 05:00:01.017 +29:59:40.48
Second-epoch image center 05:00:00.197 +29:59:30.96
Angular distance between the image centers 0.00 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 05:00:01.017 +29:59:40.48
Second-epoch image center 04:59:57.984 +29:59:21.78
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 05:00:00.197 +29:59:30.96
Second-epoch second image center 04:59:57.984 +29:59:21.78
Angular distance between the image centers 0.00838 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.AF3ayw9nFI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.gVN5XO23WU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits &> /tmp/tmp.0uo6j1EsQ7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.nfS66laTN8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
The reference image (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat) found
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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 6875 out of 129003 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.825003
a=0.000000 b=1.000000 c=22.825003
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 261 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.3 pix fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
2.3 pix fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
Limiting magnitude estimates:
15.6 mag. Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.5 mag. Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
15.3 mag. fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
15.3 mag. fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AF3ayw9nFI (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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=14027, passed=128967
Got 128967 stars (including 114720 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
util/solve_plate_with_UCAC5 got 128967 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 951 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: 0.37"
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 951 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 - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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.gVN5XO23WU (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/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=13827, passed=129020
Got 129020 stars (including 114972 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
util/solve_plate_with_UCAC5 got 129020 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 951 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: 0.38"
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 951 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: 0.38"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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.0uo6j1EsQ7 (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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=10061, passed=102366
Got 102366 stars (including 92185 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 102366 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 951 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nfS66laTN8 (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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=10118, passed=102045
Got 102045 stars (including 91800 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 102045 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Saving fully-calibrated image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-11_20.00sec_-14.90C_LIGHT_0022.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.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_Aur-05-Q2b1x1_213543_TTUQ2b1x1_3023_VAvo7UTL/wcs_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023.fits
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out139434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out18582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out37092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out151377.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out151440.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out151535.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out151991.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out07740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76531.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 89s
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: 34s
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Considering the candidate 151274_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151274_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:36:18.20 +33:44:27.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)
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Considering the candidate 151297_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151297_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151301_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151301_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:41.25 +30:38:54.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)
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Considering the candidate 151303_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151303_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:10:47.13 +31:22:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.190 180504594846380160 077.69651828685 +31.37768182676 14.8305 13.9941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151305_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151305_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151312_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151312_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:29:18.83 +33:29:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 3.633 172906896482350464 067.32725607233 +33.48805196688 13.5880 12.7903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151314_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151314_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:32:23.27 +28:04:13.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)
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Considering the candidate 151315_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151315_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:54:09.01 +33:37:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.304 161629205716795008 073.53758618528 +33.61770191821 14.1804 13.4809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151316_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151316_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:26:25.93 +30:05:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 3.496 3446943531170648576 081.60736830168 +30.09774923134 14.4545 13.7963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151321_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151321_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:29:57.32 +34:47:48.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)
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Considering the candidate 151324_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151324_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:28:03.58 +26:43:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.722 3418155361816369536 082.01504538897 +26.72952555500 14.2394 13.4538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151325_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151325_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:25.41 +34:14:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 3.970 173200951419235328 066.10706794561 +34.24152116822 13.3640 12.5719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151326_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151326_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:47:34.57 +28:48:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.932 158197737301546496 071.89495728782 +28.80844518702 14.0931 13.1755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151327_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151327_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:55.24 +33:03:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 0.158 172694901192764928 066.23019314815 +33.05792662894 13.5763 12.9825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151330_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151330_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:35:19.72 +29:36:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.096 3445968161276710784 083.83282355622 +29.61197392681 14.0472 13.2483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151336_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151336_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:22:31.65 +29:32:34.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)
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Considering the candidate 151349_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151349_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:29:51.96 +34:19:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 3.120 182596828038249984 082.46731339244 +34.32399222199 14.2696 13.7104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151354_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151354_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:03:38.12 +28:31:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.106 155513863777579904 075.90916033275 +28.52811373070 13.8279 12.8245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151356_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151356_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 151358_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151358_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:09:09.95 +34:10:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.416 184834677796537856 077.29191302119 +34.18211120135 14.7591 14.1127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151360_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151360_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:35:29.24 +33:01:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.626 3448886677454050176 083.87236882767 +33.02032668671 13.7443 12.8407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151363_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151363_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:33.02 +31:06:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.440 171489802088658432 066.38863201108 +31.10781213052 13.6636 12.7402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151368_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151368_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:27:37.20 +32:45:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 4.051 172460803998384640 066.90379135854 +32.75543394860 13.4352 12.7698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151373_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151373_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:16.25 +33:36:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.040 172791795654832128 066.06674552000 +33.60595764668 13.1368 12.4708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151374_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151374_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:17:26.73 +25:03:51.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)
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Considering the candidate 151375_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151375_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 151376_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151376_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151377_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151377_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:30:43.15 +24:36:50.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)
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Considering the candidate 151378_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151378_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:43.12 +34:49:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 5.343 173245481640068992 066.67809181283 +34.82767346320 13.1752 12.5105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151379_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151379_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 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 151381_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151381_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:21.41 +32:54:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.063 172498775805908736 066.33885688902 +32.90034066723 13.4865 12.9605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151382_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151382_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:00.00 +33:11:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 5.056 172706441768394624 066.00166986090 +33.18830621550 13.0439 12.2833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151383_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151383_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:38.67 +32:13:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 4.842 172314328434864000 066.65958683299 +32.21660480029 13.3225 12.7038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151384_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151384_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:28:47.58 +33:09:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.620 172848935900133248 067.19720372278 +33.15231173273 13.5505 12.9752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151385_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151385_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:18:32.06 +29:23:05.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)
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Considering the candidate 151389_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151389_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:27:45.72 +33:11:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 4.154 172524717408249472 066.94186995533 +33.20007712264 13.5402 12.8474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151394_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151394_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 151400_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151400_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:28:46.43 +32:56:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.243 172468298718322304 067.19452863688 +32.94540063349 13.4544 12.8296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151401_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151401_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:27:41.44 +34:12:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 3.360 173164908053812992 066.92377848448 +34.21075604259 13.1952 12.4911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151404_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151404_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 151405_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151405_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151406_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151406_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:28:00.12 +34:40:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 4.702 173228915949835776 067.00201018989 +34.67857107802 13.0682 12.4283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151407_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151407_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151411_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151411_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151412_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151412_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 151414_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151414_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:21.52 +31:44:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 5.840 172283202807233408 066.08776393205 +31.73416450858 13.0299 12.3827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151415_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151415_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:16:24.76 +33:19:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 2.596 181870188288971520 079.10390771511 +33.32261947484 14.0510 13.6249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151416_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151416_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151417_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151417_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:06.31 +33:21:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 5.350 172724003891028736 066.52455695209 +33.35380270174 12.8685 12.2279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151420_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151420_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:36:17.89 +33:15:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 3.177 3449265729790823680 084.07559682481 +33.26243273028 13.7127 12.8368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151421_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151421_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:08.62 +25:03:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.406 149641372174991104 066.53706228980 +25.05756529733 13.2547 12.5321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151422_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151422_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:32:51.49 +34:54:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.056 173106771376570496 068.21331245417 +34.90986415941 13.2192 12.5265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151424_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151424_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 151425_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151425_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:06.14 +30:58:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.818 165482585950162688 066.27648931291 +30.97370757779 13.2720 12.6147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151426_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151426_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 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 151428_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151428_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151429_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151429_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151434_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151434_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151436_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151436_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:27:12.71 +25:37:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.417 151166704038840192 066.80339472604 +25.61859197750 13.4760 12.5036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151437_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151437_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 151440_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151440_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:09.43 +32:37:54.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)
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Considering the candidate 151443_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151443_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 151444_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151444_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151449_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151449_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:16:05.79 +25:21:42.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)
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Considering the candidate 151452_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151452_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151453_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151453_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:02:17.55 +26:48:50.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)
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Considering the candidate 151454_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151454_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:58.81 +25:20:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.285 151153235021421696 066.74541585903 +25.34033044651 13.2685 12.5322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151456_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151456_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:21.11 +25:32:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.108 151170964646329856 066.58917948339 +25.53574141020 13.2009 12.4265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151459_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151459_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 151461_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151461_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:16.59 +33:35:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 5.004 172744928971658368 066.31745680714 +33.59552145417 12.8973 12.1400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151462_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151462_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:23:38.00 +33:46:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.212 172809314825100416 065.90940419332 +33.77571745090 12.8543 12.0432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151464_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151464_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:08.47 +32:20:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.706 172377863886052480 066.28549711694 +32.34674220915 13.0652 12.4034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151466_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151466_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151469_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151469_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151470_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151470_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 151471_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151471_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:31.49 +32:39:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 3.763 172401400306797952 066.13004792941 +32.65754496300 12.9959 12.3046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151473_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151473_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151475_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151475_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 151479_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151479_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:38.28 +32:14:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.289 172329240561314432 066.40842662584 +32.24040681529 12.9760 12.3229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151480_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151480_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151485_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151485_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151486_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151486_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151487_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151487_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151488_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151488_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 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 151490_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151490_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151491_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151491_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:30:52.73 +34:22:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.524 173068627770091264 067.72140051703 +34.37477420763 12.8959 12.1695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151494_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151494_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:19.32 +34:47:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.174 176241715249554816 066.58168205260 +34.79796762779 12.7918 11.9223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151495_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151495_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:34:45.36 +34:10:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.923 3449510615944158848 083.68963615678 +34.17648053439 13.3932 12.4480 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 151496_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151496_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:28.91 +33:53:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.043 172816981342803072 066.11877081597 +33.89922819227 12.7105 12.0894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151500_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151500_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:11.64 +33:53:18.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 151501_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151501_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151503_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151503_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151505_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151505_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:32.80 +28:13:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.453 152860192463932672 066.63676008098 +28.22551584306 12.9917 12.2164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151506_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151506_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151511_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151511_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:27:25.06 +33:13:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 5.730 172535953042700544 066.85611177431 +33.22619501007 12.7638 12.1225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151513_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151513_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151516_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151516_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:28:24.17 +33:07:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.487 172520521223641600 067.10114387302 +33.11736072637 12.5857 11.7980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151517_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151517_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151523_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151523_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151525_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151525_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151527_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151527_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 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 151528_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151528_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:22.93 +34:04:00.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 151529_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151529_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151531_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151531_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:53.11 +30:59:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.073 165436509540982784 066.47188703279 +30.98414990356 12.7527 12.1025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151532_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151532_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151534_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151534_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151535_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151535_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:31:12.53 +34:27:15.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 151538_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151538_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151540_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151540_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151541_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151541_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 151543_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151543_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:26.71 +32:46:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.499 172494029867289984 066.36308050952 +32.77846146430 12.5127 11.9412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151544_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151544_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151548_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151548_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:30:02.82 +34:11:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.469 172966033888094336 067.51357685796 +34.18468254562 12.7088 12.1773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151551_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151551_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:25.60 +32:45:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.459 172403079639701376 066.10807453014 +32.75780798604 12.5659 11.9733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151552_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151552_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:31.60 +34:49:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.366 176247762563504896 066.63022207154 +34.83200421077 12.4397 11.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151553_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151553_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:28:30.38 +33:06:56.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)
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Considering the candidate 151555_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151555_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 151560_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151560_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 151561_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151561_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151562_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151562_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:56.74 +34:22:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.129 173217306654810624 066.73549089033 +34.37891403596 12.3067 11.6762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151563_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151563_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:27.19 +32:37:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.457 172479087676138624 066.36506002226 +32.62583712898 12.3149 11.6777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151564_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151564_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151566_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151566_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:33:29.33 +34:33:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.566 173082852702247424 068.37135225361 +34.56049295288 12.5101 11.8866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151568_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151568_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 151569_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151569_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:13.87 +33:14:43.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 151575_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151575_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:17:22.34 +33:12:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.822 181115781575088768 079.34413996306 +33.20113264494 11.9382 11.2029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151577_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151577_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:27.79 +31:33:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.799 171520309240574080 066.36521329734 +31.56063814526 12.4576 11.8037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151580_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151580_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151583_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151583_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 151585_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151585_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:08.29 +32:22:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.226 172378718583396992 066.28592505560 +32.37160877919 12.2390 11.6557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151586_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151586_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151591_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151591_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:22.77 +32:38:58.4 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 151592_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151592_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:28:09.57 +25:13:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.857 150961026644282496 067.04064133712 +25.22316422264 12.7461 12.0840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151593_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151593_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 151594_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151594_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:23:48.86 +32:50:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.045 172594910057754240 065.95475842815 +32.84311959592 12.1151 11.3101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151595_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151595_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 151596_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151596_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 151597_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151597_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151598_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151598_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:25:35.63 +31:27:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.915 171516190367453824 066.39755541791 +31.45019496812 12.0888 11.5471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151600_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151600_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:28:48.70 +34:30:15.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
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Considering the candidate 151602_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151602_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151603_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151603_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:06.65 +32:36:42.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 151604_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151604_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 151606_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151606_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:29.24 +32:43:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 5.506 172484237339953792 066.62001534693 +32.72640521636 11.8702 11.2866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151607_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151607_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 151608_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151608_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 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 151610_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151610_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:07.38 +32:55:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 2.763 172689437994424704 066.03001519413 +32.92553994088 11.6984 11.1329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151614_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151614_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151616_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151616_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151618_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151618_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 151619_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151619_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:50.37 +33:29:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 5.437 172742691292340096 066.20810719484 +33.49186656844 11.2205 10.6524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151620_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151620_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 151621_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151621_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:35:46.84 +32:32:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.768 3448811773224818304 083.94569639233 +32.54953755780 10.9205 9.6706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151623_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151623_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:31:50.80 +34:50:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 2.779 173293207316591232 067.96077821681 +34.84553140041 10.7292 10.1513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151624_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151624_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:09.40 +34:09:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 3.546 173190712217394432 066.54028979965 +34.15986825057 10.3691 9.6886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151625_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151625_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:24:03.72 +31:59:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 4.257 172297118499989760 066.01410581877 +31.99766124947 10.3418 9.7347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151631_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151631_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:56:57.79 +33:05:59.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 151632_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151632_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:41:14.09 +28:37:41.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151635_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151635_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:32:30.38 +33:45:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.015 3449168457369669760 083.12690321188 +33.75604494473 12.1187 11.3810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151636_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151636_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:18:17.95 +33:47:33.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151637_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151637_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:30.52 +25:53:48.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 151642_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151642_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:04:50.98 +25:41:30.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 151645_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151645_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:36:18.99 +34:10:43.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 151653_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151653_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:26:32.80 +28:37:18.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 151655_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151655_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:38:26.82 +26:55:00.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151667_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151667_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:51:21.90 +28:31:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.010 155132122787487872 072.84160076644 +28.52152096912 12.6812 11.9748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151668_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151668_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:59:17.60 +32:33:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.390 160653427802954240 074.82410793975 +32.55968460962 10.7019 9.3585 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151677_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151677_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:28:55.09 +32:26:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.393 3448933436759573248 082.23026906251 +32.43641178181 12.7289 12.3208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151695_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151695_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151708_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151708_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:18:28.31 +33:11:30.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 151726_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151726_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:17:12.06 +32:45:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.813 181069468946427264 079.30057785923 +32.76588405202 13.4587 12.9137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151729_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151729_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:17:10.82 +32:04:55.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 151736_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151736_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:24:36.43 +30:33:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.696 3447019156954534144 081.15231721669 +30.56417484120 12.4398 11.2769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151739_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151739_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:17:17.82 +33:11:43.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 151747_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151747_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:19:27.44 +34:00:24.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151771_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151771_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:10:31.62 +30:49:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.605 156425560781628928 077.63211988348 +30.82531270274 13.4967 12.9714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151794_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151794_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:29:46.88 +29:10:28.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151799_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151799_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:09:00.87 +33:19:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.699 181723403487101184 077.25444981855 +33.32431611456 13.6818 12.8169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151802_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151802_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:21:42.69 +34:09:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.460 182767454200970368 080.42867643233 +34.16258200243 13.2646 12.2625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151803_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151803_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:28:57.17 +32:25:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.185 3448933372340532864 082.23864621552 +32.42617597516 13.5979 13.0568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151804_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151804_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:22:00.34 +32:53:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.244 180946083126621056 080.50239369815 +32.89806702261 12.8224 10.7915 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151814_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151814_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:43:52.74 +26:43:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.069 154531381418739584 070.96980171547 +26.72018209601 13.7261 12.8625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151817_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151817_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:35.89 +31:24:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.373 171501106442492160 066.64877412243 +31.40040001212 13.5756 12.7903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151824_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151824_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:28:41.15 +33:56:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 3.754 182558448210694784 082.17270153027 +33.94054021701 13.2301 12.0567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151833_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151833_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:49:22.09 +29:33:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.867 158337718875501952 072.34295533341 +29.56306005116 13.7828 13.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151845_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151845_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:58.38 +25:07:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.776 149459677877201536 066.74278238311 +25.12371648364 13.4135 12.3367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151847_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151847_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:15:52.97 +30:28:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.695 180183915409609984 078.97146830084 +30.47583178136 13.8443 13.2675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151856_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151856_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:12:51.28 +30:44:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 4.023 180238856630671872 078.21425848046 +30.73769941959 14.2090 13.4969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151857_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151857_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:32:15.78 +34:25:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 0.856 182961831539119232 083.06593604674 +34.41893156226 13.8892 13.3613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151863_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151863_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:07:47.58 +30:15:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 3.815 156288297920954368 076.94947492561 +30.26117221281 13.6082 12.7616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151865_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151865_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:04:21.55 +28:40:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.124 155609860589825152 076.08951320694 +28.68069442462 13.8801 12.9547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151872_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151872_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:27:50.37 +33:29:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.816 182445370311470976 081.96062243254 +33.49699620535 14.0832 13.6618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151879_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151879_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:34:41.71 +31:29:53.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)
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Considering the candidate 151880_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151880_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:30:05.71 +30:28:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.470 3446313747228327936 082.52424390420 +30.46859353290 14.0245 13.3446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151881_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151881_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:03:36.89 +33:23:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.315 184681703943238016 075.90443401859 +33.39622880429 12.6410 11.2206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151882_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151882_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:32:55.55 +27:36:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.135 151835134092834176 068.23111568754 +27.60541520553 13.8259 12.8982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151883_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151883_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:29:36.12 +33:29:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.296 3449146574515744384 082.40126361215 +33.48631038542 13.6101 12.7376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151884_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151884_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:16:23.97 +30:43:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 2.695 180205665123623936 079.10074453584 +30.72784835954 14.1327 13.5809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151894_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151894_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:27:07.03 +31:46:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.157 3447380346524670080 081.77997288699 +31.78057043179 13.8853 13.2554 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 151896_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151896_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:32:59.52 +25:52:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.156 3441121788898789376 083.24858208933 +25.87851533418 13.8024 13.2821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151904_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151904_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:33:20.46 +32:18:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.400 3448699721819259520 083.33569375210 +32.30149169004 13.9277 13.2424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151906_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151906_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:24:43.75 +32:43:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.016 180891004466416640 081.18269590939 +32.72582105965 13.6771 12.7609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151916_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151916_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:38:29.44 +31:30:22.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
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Considering the candidate 151924_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151924_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:30:29.64 +33:44:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 2.125 3449157191674845824 082.62420448012 +33.73417742875 13.8887 13.1009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151928_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151928_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:47:17.05 +33:06:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 5.300 161439338098717312 071.82277808380 +33.11442251982 14.0728 13.2951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151932_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151932_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 151936_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151936_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:29:52.22 +34:01:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 5.004 182577277347214464 082.46919407430 +34.03036226598 14.0470 13.1993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151937_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151937_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151940_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151940_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:31:43.87 +32:21:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 4.328 3448744874813527168 082.93296618998 +32.35369569708 14.1654 13.5189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151943_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151943_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:49:41.48 +28:20:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.680 155119517060595584 072.42333513393 +28.33776170554 13.9738 13.2318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151947_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151947_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:13:11.00 +33:19:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 3.043 181908877354300032 078.29669278738 +33.33361271073 14.3281 13.7613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151948_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151948_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:33:45.21 +34:37:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 2.259 3449604413732600320 083.43883708533 +34.61866587863 14.0505 13.5213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151949_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 151949_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 151955_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151955_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:34:11.36 +33:58:48.4 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 151958_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151958_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:33:26.96 +30:56:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.894 171286800458682880 068.36211674218 +30.93550167494 13.7791 12.1913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151962_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151962_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:34:20.31 +32:24:25.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)
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Considering the candidate 151964_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151964_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:03:51.31 +32:23:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.648 157599225019503360 075.96384113575 +32.39673361141 13.8759 12.8211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151965_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151965_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:05:53.45 +34:01:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.747 184814611709204352 076.47320439925 +34.03198012141 14.1760 13.6585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151970_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151970_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:19:56.19 +34:13:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 4.289 182021195043576576 079.98554498437 +34.22917426133 14.1367 13.6022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151971_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151971_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:31:08.11 +31:53:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 5.213 3448657738517161216 082.78542013981 +31.89520798023 13.9030 12.6585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151977_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151977_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:18:56.62 +33:46:28.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151980_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151980_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:04:43.85 +30:15:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.795 157072627669262080 076.18328379957 +30.26490458096 14.1943 13.5218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151981_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151981_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:18:27.94 +30:23:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 4.790 3446782349637223680 079.61747459866 +30.39852378169 14.3196 13.4536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151985_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151985_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:05:52.86 +31:14:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 2.482 157283046705470080 076.47098480180 +31.24502158498 14.0199 13.2657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151986_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151986_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:26:21.06 +25:04:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 4.043 149454214678814976 066.58722556075 +25.07595447985 13.6566 12.8536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151991_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151991_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:06:28.58 +29:11:58.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)
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Considering the candidate 151995_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151995_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:17:16.60 +32:46:22.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)
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Considering the candidate 151996_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151996_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:27:02.53 +34:20:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.812 182632012410069888 081.76114844968 +34.33921407195 14.3288 13.7325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151998_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 151998_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:50:23.30 +26:02:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.582 153464889498614528 072.59634369343 +26.03931356875 14.3002 13.3711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152034_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152034_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:18:23.74 +32:16:51.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)
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Considering the candidate 152041_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152041_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:09:50.77 +32:54:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 5.487 181506765335238912 077.46288000640 +32.90194237742 14.0468 13.1332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152042_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152042_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:02:21.03 +28:21:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.764 155691263106913408 075.58846390976 +28.35068265171 14.4028 13.6507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152046_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152046_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:18:30.03 +28:38:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.370 3422372882261738240 079.62520262173 +28.63799378052 14.5989 13.9969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152047_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152047_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:56:09.66 +28:58:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 3.672 155069935958117376 074.04105531288 +28.97665113106 14.5165 13.8365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152053_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152053_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:43:36.28 +27:39:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 2.669 154657138060781184 070.90148861765 +27.66500995160 14.2127 13.3552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152059_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152059_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:45:13.90 +32:49:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 4.711 161341172325617152 071.30936447932 +32.82554566523 14.4506 13.6387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152060_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152060_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:41:16.70 +29:17:42.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)
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Considering the candidate 152084_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152084_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:31:34.34 +31:29:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 2.402 3448632896426585856 082.89273476293 +31.48676386283 14.5726 13.9393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152098_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 152098_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:18:35.22 +31:00:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 1.382 180295412760891904 079.64719671430 +31.00641517348 14.4176 13.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139818_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 139818_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:23:45.50 +34:30:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.785 176221855320797952 065.94051804858 +34.51132372807 12.7822 12.2520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 37092_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 37092_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:34:07.66 +32:41:32.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)
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Considering the candidate 148707_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 148707_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (30.7") between the two second-epoch detections
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Considering the candidate 144508_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 144508_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:10:32.21 +32:10:43.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 139434_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 139434_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:29:35.22 +26:38:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.384 151376087987961216 067.39628778250 +26.63935010902 12.8516 11.8396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57253_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 57253_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 04:38:19.75 +31:18:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 5.022 159630637173582464 069.58067559348 +31.31328347481 10.8707 9.5120 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 18582_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 18582_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:02:01.79 +33:55:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.226 184942150761586816 075.50762965516 +33.92828176484 12.3590 10.6953 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07349_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 07349_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 34197_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 34197_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:05:41.85 +32:54:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.369 181638741091160192 076.42399880855 +32.91640637690 12.9920 11.5721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 76531_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 76531_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 36697_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 36697_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
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Considering the candidate 16878_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 16878_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19055_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 19055_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 110933_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 110933_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73676_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 73676_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105568_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 105568_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:15:47.39 +26:45:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18313_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 18313_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118476_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 118476_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (31.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110738_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 110738_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07740_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 07740_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62859_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
Preparing report for the candidate 62859_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139984_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023
The candidate 139984_fd_Aur-05-Q2b1x1_2026-03-19_21-10-59_20.00sec_-15.00C_LIGHT_0023 did not pass the final checks
**** FOUND 05:26:52.91 +30:33:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.91, MAG_FAINT_SEARCH_LIMIT=11.89)GAIADR2_OUTPUT=# 1.037 3446995654893636992 081.72012934555 +30.56302483901 11.0229 10.4069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 132s
Prepared the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:10:32.21 +32:10:43.0
04:26:30.52 +25:53:48.4
05:36:19.18 +34:10:42.1
05:04:50.97 +25:41:31.1
04:23:21.08 +34:29:48.8
04:26:37.17 +27:10:15.1
04:28:00.76 +33:37:09.0
04:26:39.38 +34:18:22.2
04:25:05.12 +30:49:29.1
04:25:44.17 +32:34:37.4
04:24:01.37 +32:28:44.5
04:25:36.36 +34:14:49.5
04:25:20.39 +31:38:59.8
04:25:42.73 +33:05:28.2
04:25:32.58 +30:21:05.1
04:25:34.61 +34:09:16.1
04:23:58.12 +32:46:56.8
04:25:54.39 +34:07:07.1
04:26:58.85 +33:16:03.0
04:24:00.59 +33:17:53.2
04:25:07.37 +33:57:30.0
04:26:33.27 +34:20:32.3
04:28:07.70 +34:28:18.2
04:24:53.81 +33:22:54.0
04:28:59.89 +34:49:15.1
04:24:53.05 +33:24:42.2
04:28:08.59 +33:46:22.2
04:28:11.25 +34:11:28.7
04:24:11.27 +32:49:38.1
04:25:49.16 +33:41:44.5
04:24:38.61 +33:28:25.7
04:24:00.75 +33:42:14.1
04:26:16.71 +34:31:04.8
04:23:51.46 +32:37:16.0
04:25:01.94 +34:20:42.9
04:23:35.93 +34:29:20.8
04:26:54.25 +32:49:03.7
04:27:14.44 +34:37:45.8
04:27:03.57 +34:40:41.3
04:24:36.16 +34:21:29.7
04:25:02.94 +34:52:58.8
04:27:12.93 +33:58:44.5
04:26:26.58 +33:42:15.9
04:24:24.79 +30:11:53.2
04:27:19.45 +33:41:49.8
04:28:26.03 +34:28:50.8
04:25:58.95 +33:48:03.4
05:18:46.35 +31:05:53.0
05:15:27.28 +30:39:39.4
05:20:28.19 +30:16:23.6
05:10:41.79 +33:57:11.7
05:13:11.24 +33:50:53.4
04:37:39.60 +32:37:26.1
04:49:21.32 +30:55:35.5
05:16:37.50 +29:52:08.8
########### Completed Aur-05-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:10:32.21 +32:10:43.0
04:26:30.52 +25:53:48.4
05:36:19.18 +34:10:42.1
05:04:50.97 +25:41:31.1
04:28:00.76 +33:37:09.0
04:26:39.38 +34:18:22.2
04:25:05.12 +30:49:29.1
04:25:44.17 +32:34:37.4
04:24:01.37 +32:28:44.5
04:25:36.36 +34:14:49.5
04:25:20.39 +31:38:59.8
04:25:42.73 +33:05:28.2
04:25:32.58 +30:21:05.1
04:25:34.61 +34:09:16.1
04:23:58.12 +32:46:56.8
04:25:54.39 +34:07:07.1
04:26:58.85 +33:16:03.0
04:24:00.59 +33:17:53.2
04:25:07.37 +33:57:30.0
04:26:33.27 +34:20:32.3
04:28:07.70 +34:28:18.2
04:24:53.81 +33:22:54.0
04:28:59.89 +34:49:15.1
04:24:53.05 +33:24:42.2
04:28:08.59 +33:46:22.2
04:28:11.25 +34:11:28.7
04:24:11.27 +32:49:38.1
04:25:49.16 +33:41:44.5
04:24:38.61 +33:28:25.7
04:24:00.75 +33:42:14.1
04:26:16.71 +34:31:04.8
04:23:51.46 +32:37:16.0
04:25:01.94 +34:20:42.9
04:23:35.93 +34:29:20.8
04:26:54.25 +32:49:03.7
04:27:14.44 +34:37:45.8
04:27:03.57 +34:40:41.3
04:24:36.16 +34:21:29.7
04:25:02.94 +34:52:58.8
04:27:12.93 +33:58:44.5
04:26:26.58 +33:42:15.9
04:24:24.79 +30:11:53.2
04:27:19.45 +33:41:49.8
04:28:26.03 +34:28:50.8
04:25:58.95 +33:48:03.4
05:18:46.35 +31:05:53.0
05:15:27.28 +30:39:39.4
05:20:28.19 +30:16:23.6
05:16:37.50 +29:52:08.8
04:37:39.60 +32:37:26.1
05:10:41.79 +33:57:11.7
04:26:37.17 +27:10:15.1
05:13:11.24 +33:50:53.4
04:23:21.08 +34:29:48.8
04:49:21.32 +30:55:35.5
###################################################################################
05:10:32.21 +32:10:43.0 -- not an asteroid (will add it to exclusion list)
04:26:30.52 +25:53:48.4 -- not an asteroid (will add it to exclusion list)
05:36:19.18 +34:10:42.1 -- not an asteroid (will add it to exclusion list)
05:04:50.97 +25:41:31.1 -- asteroid (will NOT add it to exclusion list)
04:28:00.76 +33:37:09.0 -- not an asteroid (will add it to exclusion list)
04:26:39.38 +34:18:22.2 -- not an asteroid (will add it to exclusion list)
04:25:05.12 +30:49:29.1 -- not an asteroid (will add it to exclusion list)
04:25:44.17 +32:34:37.4 -- not an asteroid (will add it to exclusion list)
04:24:01.37 +32:28:44.5 -- not an asteroid (will add it to exclusion list)
04:25:36.36 +34:14:49.5 -- not an asteroid (will add it to exclusion list)
04:25:20.39 +31:38:59.8 -- not an asteroid (will add it to exclusion list)
04:25:42.73 +33:05:28.2 -- not an asteroid (will add it to exclusion list)
04:25:32.58 +30:21:05.1 -- not an asteroid (will add it to exclusion list)
04:25:34.61 +34:09:16.1 -- not an asteroid (will add it to exclusion list)
04:23:58.12 +32:46:56.8 -- not an asteroid (will add it to exclusion list)
04:25:54.39 +34:07:07.1 -- not an asteroid (will add it to exclusion list)
04:26:58.85 +33:16:03.0 -- not an asteroid (will add it to exclusion list)
04:24:00.59 +33:17:53.2 -- not an asteroid (will add it to exclusion list)
04:25:07.37 +33:57:30.0 -- not an asteroid (will add it to exclusion list)
04:26:33.27 +34:20:32.3 -- not an asteroid (will add it to exclusion list)
04:28:07.70 +34:28:18.2 -- not an asteroid (will add it to exclusion list)
04:24:53.81 +33:22:54.0 -- not an asteroid (will add it to exclusion list)
04:28:59.89 +34:49:15.1 -- not an asteroid (will add it to exclusion list)
04:24:53.05 +33:24:42.2 -- not an asteroid (will add it to exclusion list)
04:28:08.59 +33:46:22.2 -- not an asteroid (will add it to exclusion list)
04:28:11.25 +34:11:28.7 -- not an asteroid (will add it to exclusion list)
04:24:11.27 +32:49:38.1 -- not an asteroid (will add it to exclusion list)
04:25:49.16 +33:41:44.5 -- not an asteroid (will add it to exclusion list)
04:24:38.61 +33:28:25.7 -- not an asteroid (will add it to exclusion list)
04:24:00.75 +33:42:14.1 -- not an asteroid (will add it to exclusion list)
04:26:16.71 +34:31:04.8 -- not an asteroid (will add it to exclusion list)
04:23:51.46 +32:37:16.0 -- not an asteroid (will add it to exclusion list)
04:25:01.94 +34:20:42.9 -- not an asteroid (will add it to exclusion list)
04:23:35.93 +34:29:20.8 -- not an asteroid (will add it to exclusion list)
04:26:54.25 +32:49:03.7 -- not an asteroid (will add it to exclusion list)
04:27:14.44 +34:37:45.8 -- not an asteroid (will add it to exclusion list)
04:27:03.57 +34:40:41.3 -- not an asteroid (will add it to exclusion list)
04:24:36.16 +34:21:29.7 -- not an asteroid (will add it to exclusion list)
04:25:02.94 +34:52:58.8 -- not an asteroid (will add it to exclusion list)
04:27:12.93 +33:58:44.5 -- not an asteroid (will add it to exclusion list)
04:26:26.58 +33:42:15.9 -- not an asteroid (will add it to exclusion list)
04:24:24.79 +30:11:53.2 -- not an asteroid (will add it to exclusion list)
04:27:19.45 +33:41:49.8 -- not an asteroid (will add it to exclusion list)
04:28:26.03 +34:28:50.8 -- not an asteroid (will add it to exclusion list)
04:25:58.95 +33:48:03.4 -- not an asteroid (will add it to exclusion list)
05:18:46.35 +31:05:53.0 -- asteroid (will NOT add it to exclusion list)
05:15:27.28 +30:39:39.4 -- not an asteroid (will add it to exclusion list)
05:20:28.19 +30:16:23.6 -- asteroid (will NOT add it to exclusion list)
05:16:37.50 +29:52:08.8 -- not an asteroid (will add it to exclusion list)
04:37:39.60 +32:37:26.1 -- not an asteroid (will add it to exclusion list)
05:10:41.79 +33:57:11.7 -- not an asteroid (will add it to exclusion list)
04:26:37.17 +27:10:15.1 -- not an asteroid (will add it to exclusion list)
05:13:11.24 +33:50:53.4 -- not an asteroid (will add it to exclusion list)
04:23:21.08 +34:29:48.8 -- not an asteroid (will add it to exclusion list)
04:49:21.32 +30:55:35.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:23:21.08 +34:29:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:35.93 +34:29:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:51.46 +32:37:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:58.12 +32:46:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:00.59 +33:17:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:00.75 +33:42:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:01.37 +32:28:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:11.27 +32:49:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:24.79 +30:11:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:36.16 +34:21:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:38.61 +33:28:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:53.05 +33:24:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:53.81 +33:22:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:01.94 +34:20:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:02.94 +34:52:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:05.12 +30:49:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:07.37 +33:57:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:20.39 +31:38:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:32.58 +30:21:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:34.61 +34:09:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:36.36 +34:14:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:42.73 +33:05:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:44.17 +32:34:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:49.16 +33:41:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:54.39 +34:07:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:58.95 +33:48:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:16.71 +34:31:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:26.58 +33:42:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:30.52 +25:53:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:33.27 +34:20:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:37.17 +27:10:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:39.38 +34:18:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:54.25 +32:49:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:58.85 +33:16:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:03.57 +34:40:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:12.93 +33:58:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:14.44 +34:37:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:19.45 +33:41:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:00.76 +33:37:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:07.70 +34:28:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:08.59 +33:46:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:11.25 +34:11:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:26.03 +34:28:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:59.89 +34:49:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:39.60 +32:37:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:21.32 +30:55:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:32.21 +32:10:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:41.79 +33:57:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:11.24 +33:50:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:27.28 +30:39:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:37.50 +29:52:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:19.18 +34:10:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
04:23:21.08 +34:29:48.8 -- a known variable star
04:23:35.93 +34:29:20.8 -- not a known variable star
04:23:51.46 +32:37:16.0 -- not a known variable star
04:23:58.12 +32:46:56.8 -- not a known variable star
04:24:00.59 +33:17:53.2 -- a known variable star
04:24:00.75 +33:42:14.1 -- not a known variable star
04:24:01.37 +32:28:44.5 -- not a known variable star
04:24:11.27 +32:49:38.1 -- a known variable star
04:24:24.79 +30:11:53.2 -- not a known variable star
04:24:36.16 +34:21:29.7 -- not a known variable star
04:24:38.61 +33:28:25.7 -- not a known variable star
04:24:53.05 +33:24:42.2 -- not a known variable star
04:24:53.81 +33:22:54.0 -- not a known variable star
04:25:01.94 +34:20:42.9 -- not a known variable star
04:25:02.94 +34:52:58.8 -- a known variable star
04:25:05.12 +30:49:29.1 -- not a known variable star
04:25:07.37 +33:57:30.0 -- not a known variable star
04:25:20.39 +31:38:59.8 -- not a known variable star
04:25:32.58 +30:21:05.1 -- a known variable star
04:25:34.61 +34:09:16.1 -- not a known variable star
04:25:36.36 +34:14:49.5 -- not a known variable star
04:25:42.73 +33:05:28.2 -- not a known variable star
04:25:44.17 +32:34:37.4 -- not a known variable star
04:25:49.16 +33:41:44.5 -- not a known variable star
04:25:54.39 +34:07:07.1 -- not a known variable star
04:25:58.95 +33:48:03.4 -- not a known variable star
04:26:16.71 +34:31:04.8 -- not a known variable star
04:26:26.58 +33:42:15.9 -- not a known variable star
04:26:30.52 +25:53:48.4 -- a known variable star
04:26:33.27 +34:20:32.3 -- not a known variable star
04:26:37.17 +27:10:15.1 -- not a known variable star
04:26:39.38 +34:18:22.2 -- not a known variable star
04:26:54.25 +32:49:03.7 -- not a known variable star
04:26:58.85 +33:16:03.0 -- not a known variable star
04:27:03.57 +34:40:41.3 -- not a known variable star
04:27:12.93 +33:58:44.5 -- not a known variable star
04:27:14.44 +34:37:45.8 -- not a known variable star
04:27:19.45 +33:41:49.8 -- not a known variable star
04:28:00.76 +33:37:09.0 -- not a known variable star
04:28:07.70 +34:28:18.2 -- not a known variable star
04:28:08.59 +33:46:22.2 -- not a known variable star
04:28:11.25 +34:11:28.7 -- not a known variable star
04:28:26.03 +34:28:50.8 -- not a known variable star
04:28:59.89 +34:49:15.1 -- not a known variable star
04:37:39.60 +32:37:26.1 -- a known variable star
04:49:21.32 +30:55:35.5 -- a known variable star
05:10:32.21 +32:10:43.0 -- a known variable star
05:10:41.79 +33:57:11.7 -- a known variable star
05:13:11.24 +33:50:53.4 -- a known variable star
05:15:27.28 +30:39:39.4 -- not a known variable star
05:16:37.50 +29:52:08.8 -- a known variable star
05:36:19.18 +34:10:42.1 -- a known variable star
Found 39 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
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52 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 52 (excluding asteroids and hot pixels), not updating the exclusion list!
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Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461119.59052963 -observatory 500
22:37:26.89 -07:25:57.8 Mercury (1.2mag)
01:02:26.32 +05:41:26.5 Venus (-3.9mag)
23:00:30.61 -07:30:56.6 Mars (1.2mag)
07:04:38.60 +22:58:09.1 Jupiter (-2.3mag)
00:16:55.96 -00:28:52.0 Saturn (0.9mag)
03:42:47.95 +19:31:25.0 Uranus (5.8mag)
00:07:09.80 -00:38:51.2 Neptune (7.8mag)
20:31:55.42 -22:53:55.2 Pluto (14.5mag)
00:41:55.10 +07:42:18.9 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Mar 19 21:43 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461119.59052963:
07:04:29.60 +22:58:25.7 Io (5.6mag)
07:04:41.54 +22:57:59.8 Europa (5.7mag)
07:04:29.23 +22:58:18.9 Ganymede (5.2mag)
07:04:10.12 +22:58:53.6 Callisto (6.4mag)
07:08:40.04 +23:00:17.9 Himalia (15.2mag)
07:04:37.55 +22:58:08.2 Thebe (16.0mag)
07:08:13.80 +23:23:10.2 Elara (17.1mag)
07:01:43.08 +23:52:19.1 Pasiphae (17.2mag)
07:13:26.76 +22:52:26.4 Carme (18.3mag)
00:16:47.73 -00:28:41.0 Titan (8.8mag)
00:16:55.13 -00:28:46.5 Rhea (10.1mag)
00:17:26.39 -00:26:53.6 Iapetus (11.5mag)
00:17:10.05 -00:29:00.5 Hyperion (14.8mag)
00:18:50.58 -00:17:31.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 19 21:43 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461119.59052963:
12:42:14.48 +09:48:49.8 JWST
19:20:00.76 +12:48:18.2 Chandra
15:25:10.68 -59:15:12.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 19 21:43 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461119.59052963 -observatory 500
18:34:38.12 -27:25:18.0 14.1mag P/2010 H2 (Vales)
04:50:44.70 -71:05:07.5 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:40.84 +31:17:41.0 17.0mag C/2017 K2 (PANSTARRS)
17:29:28.97 +07:17:44.8 17.6mag C/2021 G2 (ATLAS)
23:01:12.10 +28:25:07.7 16.9mag C/2022 E2 (ATLAS)
03:59:33.44 +25:16:05.0 15.7mag C/2022 N2 (PANSTARRS)
09:01:58.84 +31:24:44.6 16.0mag C/2022 QE78 (ATLAS)
08:30:16.60 -03:17:26.6 17.2mag C/2022 R6 (PANSTARRS)
18:56:28.25 +16:12:49.9 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:26.68 -11:51:13.4 17.6mag P/2023 B1 (PANSTARRS)
09:25:17.77 -16:29:17.9 17.4mag C/2023 F3 (ATLAS)
21:20:19.80 +61:40:01.1 17.4mag C/2023 H5 (Lemmon)
19:33:25.53 -03:31:03.8 14.5mag C/2023 R1 (PANSTARRS)
21:35:34.22 +82:46:23.7 17.7mag C/2023 X2 (Lemmon)
06:15:42.81 +63:47:54.0 16.8mag C/2024 A1 (ATLAS)
04:03:27.41 +04:31:05.5 9.0mag C/2024 E1 (Wierzchos)
11:23:23.56 +02:33:01.8 18.0mag C/2024 G2 (ATLAS)
16:32:35.19 +02:01:20.2 17.5mag C/2024 G6 (ATLAS)
20:09:34.32 +08:33:26.6 14.9mag C/2024 J3 (ATLAS)
03:04:00.98 -26:48:47.7 16.5mag C/2024 T5 (ATLAS)
04:57:00.70 +52:53:49.2 17.6mag C/2025 J1 (Borisov)
15:16:12.06 +16:14:15.9 14.4mag C/2025 L1 (ATLAS)
02:47:23.80 -22:27:44.4 17.6mag C/2025 Q3 (ATLAS)
22:32:19.86 +18:57:09.8 12.6mag C/2025 R3 (PANSTARRS)
13:05:24.67 +01:15:06.2 17.7mag C/2025 Y1 (ATLAS)
02:12:00.28 -06:54:23.1 14.3mag C/2026 A1 (MAPS)
22:35:50.75 +30:46:03.2 13.7mag C/2026 B2 (Sun-Gao)
17:50:17.61 -10:52:00.6 13.4mag 10P/Tempel
15:27:12.60 +05:10:59.1 11.7mag 24P/Schaumasse
11:12:22.85 -02:30:58.1 15.6mag 29P/Schwassmann-Wachmann
17:42:43.20 -10:40:47.6 17.3mag 40P/Vaisala
10:45:38.02 -06:39:35.1 16.4mag 43P/Wolf-Harrington
01:07:35.46 +12:45:33.5 17.0mag 47P/Ashbrook-Jackson
06:27:22.56 +42:31:45.6 17.1mag 63P/Wild
22:52:55.19 -14:51:44.3 15.7mag 65P/Gunn
02:56:21.74 +10:56:34.6 15.9mag 76P/West-Kohoutek-Ikemura
00:07:36.22 +02:52:03.0 14.7mag 78P/Gehrels
21:35:35.97 -16:58:36.9 14.5mag 88P/Howell
00:58:27.97 +12:57:19.6 15.3mag 93P/Lovas
04:09:14.62 +30:37:27.6 16.5mag 123P/West-Hartley
08:07:33.21 +50:40:12.2 16.2mag 124P/Mrkos
01:53:01.78 +11:14:45.1 16.4mag 128P/Shoemaker-Holt
01:55:40.83 +10:54:11.1 17.4mag 131P/Mueller
23:16:07.13 +02:44:07.8 13.1mag 141P/Machholz
23:26:11.10 -04:43:14.8 13.1mag 141P-A/Machholz
22:27:31.61 -07:12:03.6 16.2mag 141P-D/Machholz
23:47:53.06 -14:33:54.7 15.5mag 162P/SidingSpring
10:39:59.59 +32:02:14.6 17.5mag 164P/Christensen
05:48:10.41 +24:44:28.6 17.5mag 198P/ODAS
15:34:29.82 -03:29:55.3 16.9mag 210P/Christensen
20:08:20.09 -17:44:20.5 17.1mag 218P/LINEAR
16:58:17.90 -16:45:11.3 16.3mag 235P/LINEAR
04:39:43.35 +31:52:43.6 16.3mag 240P/NEAT
07:29:44.84 -08:29:51.5 17.5mag 242P/Spahr
15:48:36.98 +05:02:11.6 17.7mag 391P/Kowalski
07:27:55.40 +21:05:30.5 17.5mag 450P/LONEOS
04:59:52.10 +46:40:36.7 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 19 21:43 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
-rw-r--r-- 1 apache apache 5.7K Mar 19 21:43 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 19 21:43 tocp_transients_list.txt
