This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6223,11.52,0.05,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
VARIABLE_NAME 20260329.1223 11.52CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:44.72 +11:17:02.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 04 11.35 +12 35 21.9 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3342735010247426944,2461128.6223,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3342735010247426944 20260329.1223 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:11.35 +12:35:21.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 14 35.48 +11 15 30.7 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3330124509527956224,2461128.6223,14.26,0.05,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 3330124509527956224 20260329.1223 14.26CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:35.48 +11:15:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 01 33.03 +12 58 52.5 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:33.03 +12:58:52.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.42 06:13:19.53 +14:42:59.0
195.52250 -1.52725 galactic Ori Second-epoch detections are separated by 3.6" 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 | ATO J093.3340+14.7248 | 06:13:21.05 +14:43:11.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 13 19.53 +14 42 59.0 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3340+14.7248,2461128.6223,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J093.3340+14.7248 20260329.1223 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:19.53 +14:42:59.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.33 06:11:39.40 +15:01:29.1
195.05836 -1.73323 galactic Ori Second-epoch detections are separated by 1.7" 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 J092.9136+15.0194 | 06:11:39.40 +15:01:29.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 11 39.40 +15 01 29.1 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.9136+15.0194,2461128.6223,14.33,0.05,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 J092.9136+15.0194 20260329.1223 14.33CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:39.40 +15:01:29.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.45 06:00:51.32 +16:19:51.9
192.64943 -3.36857 galactic Ori Second-epoch detections are separated by 1.1" 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 | Gaia DR3 3348904713587288576 | 06:00:51.55 +16:19:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 00 51.32 +16 19 51.9 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348904713587288576,2461128.6223,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3348904713587288576 20260329.1223 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:51.32 +16:19:51.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.38 06:08:32.34 +12:55:13.0
196.54022 -3.40937 galactic Ori Second-epoch detections are separated by 3.1" 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 | 06:08:32.34 +12:55:13.0 (user input) | T | P | (position from user input) SpType: G0 (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 29.1223* 06 08 32.34 +12 55 13.0 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.38,0.05,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 20260329.1223 14.38CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:32.34 +12:55:13.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.20 06:15:54.44 +12:55:37.6
197.39486 -1.82990 galactic Ori Second-epoch detections are separated by 4.4" 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 J093.9813+12.9273 | 06:15:54.44 +12:55:37.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 15 54.44 +12 55 37.6 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.9813+12.9273,2461128.6223,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J093.9813+12.9273 20260329.1223 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:54.44 +12:55:37.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 58 30.36 +17 12 37.4 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:30.36 +17:12:37.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 58 29.54 +15 03 34.6 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:29.54 +15:03:34.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.10 06:28:29.58 +15:24:33.8
196.63619 2.02902 galactic Gem Second-epoch detections are separated by 1.0" 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 J097.1233+15.4037 | 06:28:29.58 +15:24:33.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J097.1233+15.4037,2461128.6223,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.1233+15.4037 20260329.1223 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:29.58 +15:24:33.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 11 23.33 +15 36 18.7 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:23.33 +15:36:18.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.20 06:11:51.37 +15:43:45.7
194.46330 -1.35250 galactic Ori Second-epoch detections are separated by 1.2" 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 | Gaia DR3 3345845459921929216 | 06:11:50.48 +15:43:16.9 (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 29.1223* 06 11 51.37 +15 43 45.7 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345845459921929216,2461128.6223,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3345845459921929216 20260329.1223 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:51.37 +15:43:45.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.30 05:56:00.70 +11:46:10.3
196.05043 -6.64137 galactic Ori Second-epoch detections are separated by 1.8" 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 | ATO J089.0060+11.7605 | 05:56:00.70 +11:46:10.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.757+/-0.149 (Very red! L if it's a dwarf)
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 29.1223* 05 56 00.70 +11 46 10.3 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.0060+11.7605,2461128.6223,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.0060+11.7605 20260329.1223 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:00.70 +11:46:10.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.31 06:08:22.48 +11:49:59.2
197.47540 -3.96849 galactic Ori Second-epoch detections are separated by 3.1" 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 | ATO J092.0837+11.8247 | 06:08:22.48 +11:49:59.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 08 22.48 +11 49 59.2 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.0837+11.8247,2461128.6223,14.31,0.05,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 J092.0837+11.8247 20260329.1223 14.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:22.48 +11:49:59.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 50 15.94 +13 54 06.7 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:15.94 +13:54:06.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 11 31.89 +13 26 07.7 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.26,0.05,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 20260329.1223 14.26CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:31.89 +13:26:07.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.20 06:32:37.70 +17:57:41.0
194.82448 4.08342 galactic Gem Second-epoch detections are separated by 2.1" 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 3371261667630411520 | 06:32:37.64 +17:57:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3371261667630411520,2461128.6223,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3371261667630411520 20260329.1223 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:37.70 +17:57:41.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 50 13.32 +13 10 47.3 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3346393158450344704,2461128.6223,14.25,0.05,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 3346393158450344704 20260329.1223 14.25CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:13.32 +13:10:47.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.36 05:52:57.06 +13:18:07.9
194.33781 -6.52990 galactic Tau Second-epoch detections are separated by 1.5" 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 | ATO J088.2419+13.2985 | 05:52:57.06 +13:18:07.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 52 57.06 +13 18 07.9 14.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.2419+13.2985,2461128.6223,14.36,0.05,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
ATO J088.2419+13.2985 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:57.06 +13:18:07.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 01 37.27 +15 19 51.9 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348495248586480128,2461128.6223,14.19,0.05,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
Gaia DR3 3348495248586480128 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:37.27 +15:19:51.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.07 06:01:45.31 +11:15:08.8
197.19727 -5.66828 galactic Ori Second-epoch detections are separated by 0.6" 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 | ATO J090.4437+11.2474 | 06:01:45.31 +11:15:08.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 01 45.31 +11 15 08.8 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.4437+11.2474,2461128.6223,14.07,0.05,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 J090.4437+11.2474 20260329.1223 14.07CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:45.31 +11:15:08.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 02 38.41 +14 07 58.5 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:38.41 +14:07:58.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.14 06:31:46.63 +18:03:22.1
194.64716 3.94689 galactic Gem Second-epoch detections are separated by 1.5" 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 | ATO J097.9458+18.0543 | 06:31:46.63 +18:03:22.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.9458+18.0543,2461128.6223,14.14,0.05,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
ATO J097.9458+18.0543 20260329.1223 14.14CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:46.63 +18:03:22.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 06 13.09 +16 19 25.9 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.09,0.05,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 20260329.1223 14.09CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:13.09 +16:19:25.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 59 02.80 +14 46 12.3 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348448935957386240,2461128.6223,14.31,0.05,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 3348448935957386240 20260329.1223 14.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:02.80 +14:46:12.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.49 06:02:21.36 +16:12:34.2
192.93301 -3.11495 galactic Ori 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 | target | 06:02:21.36 +16:12:34.2 (user input) | T | P | (position from user input) SpType: G0 (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 29.1223* 06 02 21.36 +16 12 34.2 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.49,0.05,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 20260329.1223 14.49CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:21.36 +16:12:34.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 08 27.07 +16 23 02.2 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:27.07 +16:23:02.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.01,0.05,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 20260329.1223 14.01CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:27.64 +13:42:19.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.21 05:55:28.40 +12:46:35.7
195.10398 -6.25800 galactic Ori Second-epoch detections are separated by 1.3" 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 | target | 05:55:28.40 +12:46:35.7 (user input) | T | P | (position from user input) SpType: A2V (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 29.1223* 05 55 28.40 +12 46 35.7 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:28.40 +12:46:35.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 55 21.77 +15 39 09.2 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348796553430528512,2461128.6223,14.25,0.05,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 3348796553430528512 20260329.1223 14.25CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:21.77 +15:39:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.04 06:04:18.72 +12:32:52.4
196.36654 -4.49155 galactic Ori Second-epoch detections are separated by 0.7" 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 | 06:04:18.72 +12:32:52.4 (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 29.1223* 06 04 18.72 +12 32 52.4 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.04,0.05,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 20260329.1223 14.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:18.72 +12:32:52.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.20 06:09:52.59 +14:42:45.0
195.12506 -2.26056 galactic Ori Second-epoch detections are separated by 1.7" 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 | 06:09:52.59 +14:42:45.0 (user input) | T | P | (position from user input) SpType: F6 (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 29.1223* 06 09 52.59 +14 42 45.0 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:52.59 +14:42:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.22 05:52:23.63 +14:54:07.5
192.87631 -5.84670 galactic Tau Second-epoch detections are separated by 2.0" 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 | ATO J088.0908+14.9020 | 05:52:23.63 +14:54:07.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (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 29.1223* 05 52 23.63 +14 54 07.5 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.0908+14.9020,2461128.6223,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.0908+14.9020 20260329.1223 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:23.63 +14:54:07.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.11 06:26:01.11 +16:56:24.1
195.00359 2.21362 galactic Gem Second-epoch detections are separated by 2.2" 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 | 06:26:01.11 +16:56:24.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.11,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:01.11 +16:56:24.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 10 22.29 +16 14 32.2 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.96,0.05,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
target 20260329.1223 13.96CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:22.29 +16:14:32.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.93 06:34:28.25 +17:43:05.2
195.24225 4.36246 galactic Gem Second-epoch detections are separated by 1.0" 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 | ATO J098.6143+17.7229 | 06:34:28.25 +17:43:05.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) 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!
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 J098.6143+17.7229,2461128.6223,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.6143+17.7229 20260329.1223 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:28.25 +17:43:05.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 01 12.93 +14 02 43.4 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.95,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:12.93 +14:02:43.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.01 06:00:38.09 +15:37:19.4
193.24129 -3.76428 galactic Ori Second-epoch detections are separated by 1.7" 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 3348655502404916480 | 06:00:38.40 +15:36:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 00 38.09 +15 37 19.4 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348655502404916480,2461128.6223,14.01,0.05,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 3348655502404916480 20260329.1223 14.01CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:38.09 +15:37:19.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 3369437234244553984,2461128.6223,14.04,0.05,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 3369437234244553984 20260329.1223 14.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:42.38 +16:47:43.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.08 06:00:38.27 +15:56:45.7
192.95921 -3.60392 galactic Ori Second-epoch detections are separated by 2.4" 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 | Gaia DR3 3348858568458675072 | 06:00:39.09 +15:56:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5) J-Ks=0.572+/-0.093 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 00 38.27 +15 56 45.7 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348858568458675072,2461128.6223,14.08,0.05,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 3348858568458675072 20260329.1223 14.08CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:38.27 +15:56:45.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.15 06:11:44.51 +17:21:10.0
193.02643 -0.59602 galactic Ori 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 | ATO J092.9294+17.3499 | 06:11:44.51 +17:21:10.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 11 44.51 +17 21 10.0 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.9294+17.3499,2461128.6223,14.15,0.05,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
ATO J092.9294+17.3499 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:44.51 +17:21:10.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.88 06:27:07.91 +16:55:02.4
195.14753 2.43886 galactic Gem Second-epoch detections are separated by 0.4" 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 | Gaia DR3 3369585530874840448 | 06:27:07.42 +16:55:21.2 (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!
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 3369585530874840448,2461128.6223,13.88,0.05,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 3369585530874840448 20260329.1223 13.88CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:07.91 +16:55:02.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 57 44.30 +13 34 32.9 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.07,0.05,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 20260329.1223 14.07CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:44.30 +13:34:32.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.94 06:21:43.42 +12:44:20.6
198.23105 -0.66949 galactic Ori Second-epoch detections are separated by 2.2" 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 | Gaia DR3 3332188460353765376 | 06:21:42.28 +12:44:36.8 (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 29.1223* 06 21 43.42 +12 44 20.6 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3332188460353765376,2461128.6223,13.94,0.05,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
Gaia DR3 3332188460353765376 20260329.1223 13.94CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:43.42 +12:44:20.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.99 05:51:44.66 +14:17:01.2
193.33509 -6.29280 galactic Tau Second-epoch detections are separated by 0.4" 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 | target | 05:51:44.66 +14:17:01.2 (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 29.1223* 05 51 44.66 +14 17 01.2 14.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.99,0.05,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 20260329.1223 13.99CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:44.66 +14:17:01.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.95 06:07:08.68 +12:32:31.1
196.70768 -3.88979 galactic Ori Second-epoch detections are separated by 4.3" 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 | Gaia DR3 3342698692005715072 | 06:07:06.48 +12:32:33.1 (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 29.1223* 06 07 08.68 +12 32 31.1 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3342698692005715072,2461128.6223,13.95,0.05,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
Gaia DR3 3342698692005715072 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:08.68 +12:32:31.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.14 06:08:08.26 +14:27:05.4
195.15042 -2.75500 galactic Ori Second-epoch detections are separated by 1.8" 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 | 06:08:08.26 +14:27:05.4 (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 29.1223* 06 08 08.26 +14 27 05.4 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.14,0.05,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
target 20260329.1223 14.14CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:08.26 +14:27:05.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.04 06:15:50.94 +17:58:52.8
192.94282 0.56384 galactic Ori Second-epoch detections are separated by 1.5" 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 | Gaia DR3 3373374241785762944 | 06:15:49.17 +17:58:46.9 (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 29.1223* 06 15 50.94 +17 58 52.8 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3373374241785762944,2461128.6223,14.04,0.05,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 3373374241785762944 20260329.1223 14.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:50.94 +17:58:52.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 57 00.12 +13 28 56.6 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.97,0.05,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
target 20260329.1223 13.97CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:00.12 +13:28:56.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.85 06:15:32.34 +13:47:36.2
196.58994 -1.49656 galactic Ori Second-epoch detections are separated by 2.8" 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 3344563532443313024 | 06:15:31.10 +13:47:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1959ApJS....4...23M LF 8 +13 183
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 29.1223* 06 15 32.34 +13 47 36.2 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344563532443313024,2461128.6223,13.85,0.05,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 3344563532443313024 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:32.34 +13:47:36.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 13 27.53 +14 13 51.9 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344791960283157248,2461128.6223,13.89,0.05,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
Gaia DR3 3344791960283157248 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:27.53 +14:13:51.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 10 32.45 +16 29 31.2 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.03,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:32.45 +16:29:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.02 05:54:18.55 +15:25:19.1
192.65674 -5.18631 galactic Ori Second-epoch detections are separated by 1.7" 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 | ATO J088.5853+15.4312 | 05:54:18.55 +15:25:19.1 (user input) | IRR (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 29.1223* 05 54 18.55 +15 25 19.1 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.5853+15.4312,2461128.6223,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.5853+15.4312 20260329.1223 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:18.55 +15:25:19.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.05 05:54:12.38 +15:02:21.1
192.97724 -5.39912 galactic Ori Second-epoch detections are separated by 0.8" 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 3347194221391281280 | 05:54:13.79 +15:01:59.0 (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 29.1223* 05 54 12.38 +15 02 21.1 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3347194221391281280,2461128.6223,14.05,0.05,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 3347194221391281280 20260329.1223 14.05CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:12.38 +15:02:21.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.96 05:57:35.31 +17:58:56.7
190.82544 -3.22747 galactic Ori Second-epoch detections are separated by 0.3" 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 | target | 05:57:35.31 +17:58:56.7 (user input) | T | P | (position from user input) 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 29.1223* 05 57 35.31 +17 58 56.7 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.96,0.05,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
target 20260329.1223 13.96CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:35.31 +17:58:56.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 02 12.38 +12 06 06.2 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:12.38 +12:06:06.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 55 30.15 +15 07 43.0 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:30.15 +15:07:43.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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
ZTF J063824.00+163138.3,2461128.6223,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J063824.00+163138.3 20260329.1223 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:38:24.91 +16:31:42.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.82 06:07:05.39 +10:57:47.3
198.08787 -4.66348 galactic Ori Second-epoch detections are separated by 2.6" 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 3330233837919819008 | 06:07:03.89 +10:58:26.2 (Gaia DR3) | E (local) | (local) | 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 29.1223* 06 07 05.39 +10 57 47.3 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3330233837919819008,2461128.6223,13.82,0.05,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 3330233837919819008 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:05.39 +10:57:47.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.73 06:12:20.08 +10:02:02.9
199.52507 -3.97691 galactic Ori Second-epoch detections are separated by 1.0" 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 | Gaia DR3 3329889454558446464 | 06:12:20.36 +10:02:37.3 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.493+/-0.278 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 12 20.08 +10 02 02.9 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3329889454558446464,2461128.6223,13.73,0.05,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
Gaia DR3 3329889454558446464 20260329.1223 13.73CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:20.08 +10:02:02.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 01 14.33 +14 32 07.9 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.88,0.05,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 20260329.1223 13.88CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:14.33 +14:32:07.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 49 53.50 +12 29 45.4 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.08,0.05,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 20260329.1223 14.08CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:53.50 +12:29:45.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.84 06:02:09.67 +12:11:04.5
196.42835 -5.12721 galactic Ori Second-epoch detections are separated by 0.8" 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 3342638493743157888 | 06:02:08.11 +12:10:58.9 (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!
TCP 2026 03 29.1223* 06 02 09.67 +12 11 04.5 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3342638493743157888,2461128.6223,13.84,0.05,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 3342638493743157888 20260329.1223 13.84CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:09.67 +12:11:04.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 17 55.26 +14 42 53.9 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344918885156689408,2461128.6223,13.77,0.05,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 3344918885156689408 20260329.1223 13.77CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:55.26 +14:42:53.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 17 02.23 +15 48 27.1 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3369819387551077248,2461128.6223,13.94,0.05,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
Gaia DR3 3369819387551077248 20260329.1223 13.94CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:02.23 +15:48:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.85 06:20:26.34 +17:59:04.0
193.45705 1.52661 galactic Gem Second-epoch detections are separated by 0.2" 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 | ATO J095.1052+17.9857 | 06:20:26.34 +17:59:04.0 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J095.1052+17.9857,2461128.6223,13.85,0.05,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 J095.1052+17.9857 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:26.34 +17:59:04.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 15 57.83 +15 45 45.1 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345803992013403520,2461128.6223,13.91,0.05,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 3345803992013403520 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:57.83 +15:45:45.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 51 24.63 +13 40 34.6 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3346449199183243264,2461128.6223,13.85,0.05,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 3346449199183243264 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:24.63 +13:40:34.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.81 06:31:29.54 +15:00:32.2
197.32627 2.48558 galactic Gem Second-epoch detections are separated by 2.5" 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 | ATO J097.8677+15.0128 | 06:31:29.54 +15:00:32.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J097.8677+15.0128,2461128.6223,13.81,0.05,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
ATO J097.8677+15.0128 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:29.54 +15:00:32.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.85 05:54:03.01 +13:05:40.2
194.65314 -6.40131 galactic Ori Second-epoch detections are separated by 1.7" 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 | ATO J088.5150+13.0866 | 05:54:03.01 +13:05:40.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 54 03.01 +13 05 40.2 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.5150+13.0866,2461128.6223,13.85,0.05,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 J088.5150+13.0866 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:03.01 +13:05:40.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.82 05:52:22.26 +14:25:29.3
193.28876 -6.09072 galactic Tau Second-epoch detections are separated by 2.5" 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 | ATO J088.0840+14.4203 | 05:52:22.26 +14:25:29.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 52 22.26 +14 25 29.3 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.0840+14.4203,2461128.6223,13.82,0.05,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
ATO J088.0840+14.4203 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:22.26 +14:25:29.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.78 05:54:02.77 +14:48:32.4
193.15814 -5.54764 galactic Ori Second-epoch detections are separated by 0.7" 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 | ATO J088.5095+14.8046 | 05:54:02.77 +14:48:32.4 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1223* 05 54 02.77 +14 48 32.4 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.5095+14.8046,2461128.6223,13.78,0.05,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
ATO J088.5095+14.8046 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:02.77 +14:48:32.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.79 06:37:48.45 +13:57:17.5
198.96595 3.36091 galactic Gem 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 | 06:37:48.45 +13:57:17.5 (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!
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,2461128.6223,13.79,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:48.45 +13:57:17.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.84 05:55:31.00 +15:11:03.4
193.00945 -5.05266 galactic Ori Second-epoch detections are separated by 1.5" and 5.5 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 | ATO J088.8872+15.1899 | 05:55:32.23 +15:10:40.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 05 55 31.00 +15 11 03.4 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.8872+15.1899,2461128.6223,13.84,0.05,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 J088.8872+15.1899 20260329.1223 13.84CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:31.00 +15:11:03.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 03 54.47 +12 44 04.2 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3342757279655324672,2461128.6223,13.62,0.05,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
Gaia DR3 3342757279655324672 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:54.47 +12:44:04.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.85 06:03:24.37 +14:38:53.9
194.42043 -3.65966 galactic Ori Second-epoch detections are separated by 2.4" 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 | Gaia DR3 3345438846778089728 | 06:03:23.56 +14:39:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (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 29.1223* 06 03 24.37 +14 38 53.9 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345438846778089728,2461128.6223,13.85,0.05,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 3345438846778089728 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:24.37 +14:38:53.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 00 15.12 +10 00 43.1 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6223,13.68,0.05,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
VARIABLE_NAME 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:15.12 +10:00:43.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.68,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:38:17.59 +13:56:19.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.64 06:28:19.35 +16:19:07.2
195.81080 2.41401 galactic Gem Second-epoch detections are separated by 2.2" 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 | ATO J097.0749+16.3234 | 06:28:19.35 +16:19:07.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J097.0749+16.3234,2461128.6223,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.0749+16.3234 20260329.1223 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:19.35 +16:19:07.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.65 06:15:53.67 +14:10:16.5
196.29860 -1.24086 galactic Ori 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 | Gaia DR3 3344614114276769664 | 06:15:52.19 +14:09:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1959ApJS....4...23M LF 8 +14 198
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 29.1223* 06 15 53.67 +14 10 16.5 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344614114276769664,2461128.6223,13.65,0.05,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 3344614114276769664 20260329.1223 13.65CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:53.67 +14:10:16.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.66 06:25:36.63 +13:37:50.3
197.88659 0.58404 galactic Gem Second-epoch detections are separated by 1.6" and 5.5 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 3332374174738954752 | 06:25:36.49 +13:38:09.2 (Gaia DR3) | T | P | 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!
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 3332374174738954752,2461128.6223,13.66,0.05,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 3332374174738954752 20260329.1223 13.66CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:36.63 +13:37:50.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 57 33.47 +10 55 27.7 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.74,0.05,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
target 20260329.1223 13.74CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:33.47 +10:55:27.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.68 06:00:12.83 +10:48:38.6
197.39974 -6.21381 galactic Ori Second-epoch detections are separated by 1.6" 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 | ATO J090.0584+10.8014 | 06:00:14.06 +10:48:18.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 00 12.83 +10 48 38.6 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.0584+10.8014,2461128.6223,13.68,0.05,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
ATO J090.0584+10.8014 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:12.83 +10:48:38.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.72 06:32:24.25 +14:54:07.7
197.52269 2.63189 galactic Gem Second-epoch detections are separated by 0.9" 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 | ATO J098.1010+14.9004 | 06:32:23.84 +14:53:42.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.1010+14.9004,2461128.6223,13.72,0.05,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
ATO J098.1010+14.9004 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:24.25 +14:54:07.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 09 12.73 +15 40 26.2 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345947684442695168,2461128.6223,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3345947684442695168 20260329.1223 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:12.73 +15:40:26.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.60 06:41:18.37 +18:02:06.5
195.69631 5.95649 galactic Gem Second-epoch detections are separated by 2.1" 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 | ATO J100.3264+18.0333 | 06:41:18.20 +18:02:25.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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!
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 J100.3264+18.0333,2461128.6223,13.60,0.05,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 J100.3264+18.0333 20260329.1223 13.60CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:18.37 +18:02:06.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.74 06:11:23.67 +14:49:43.8
195.19980 -1.88292 galactic Ori Second-epoch detections are separated by 0.8" 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 3345638137560150272 | 06:11:21.80 +14:49:42.0 (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 29.1223* 06 11 23.67 +14 49 43.8 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345638137560150272,2461128.6223,13.74,0.05,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
Gaia DR3 3345638137560150272 20260329.1223 13.74CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:23.67 +14:49:43.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 50 05.21 +10 34 52.9 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:05.21 +10:34:52.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.81 05:52:18.21 +15:51:58.5
192.02756 -5.38128 galactic Tau Second-epoch detections are separated by 1.1" 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 | ATO J088.0732+15.8575 | 05:52:18.21 +15:51:58.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 52 18.21 +15 51 58.5 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.0732+15.8575,2461128.6223,13.81,0.05,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
ATO J088.0732+15.8575 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:18.21 +15:51:58.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.57 06:13:49.71 +12:47:05.9
197.27842 -2.34311 galactic Ori Second-epoch detections are separated by 0.8" 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 | Gaia DR3 3344068722150832640 | 06:13:50.91 +12:47:36.0 (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 29.1223* 06 13 49.71 +12 47 05.9 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344068722150832640,2461128.6223,13.57,0.05,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
Gaia DR3 3344068722150832640 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:49.71 +12:47:05.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.57 06:16:19.10 +12:58:42.3
197.39731 -1.71742 galactic Ori Second-epoch detections are separated by 0.9" 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 | 06:16:19.10 +12:58:42.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.734+/-0.156 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 16 19.10 +12 58 42.3 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.57,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:19.10 +12:58:42.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.82 06:12:48.01 +15:57:44.1
194.36796 -1.04154 galactic Ori Second-epoch detections are separated by 2.1" 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 | 06:12:48.01 +15:57:44.1 (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 29.1223* 06 12 48.01 +15 57 44.1 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.82,0.05,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
target 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:48.01 +15:57:44.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.59 06:32:06.16 +18:09:36.7
194.58995 4.06331 galactic Gem Second-epoch detections are separated by 0.3" 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 | 06:32:06.16 +18:09:36.7 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461128.6223,13.59,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:06.16 +18:09:36.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 59 04.15 +15 40 37.4 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.66,0.05,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 20260329.1223 13.66CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:04.15 +15:40:37.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 3358733080528869760,2461128.6223,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3358733080528869760 20260329.1223 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:47.79 +16:51:34.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.80 05:58:02.29 +16:49:20.9
191.88684 -3.71177 galactic Ori Second-epoch detections are separated by 2.9" 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 J089.5004+16.8281 | 05:58:02.29 +16:49:20.9 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1223* 05 58 02.29 +16 49 20.9 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5004+16.8281,2461128.6223,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.5004+16.8281 20260329.1223 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:02.29 +16:49:20.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.48 06:36:42.85 +11:12:37.7
201.28682 1.86830 galactic Mon Second-epoch detections are separated by 1.6" 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 | Gaia DR3 3327870884349215744 | 06:36:41.84 +11:12:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3327870884349215744,2461128.6223,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3327870884349215744 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:42.85 +11:12:37.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.62 05:57:29.14 +16:25:49.5
192.16184 -4.02152 galactic Ori Second-epoch detections are separated by 0.9" 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 | ATO J089.3694+16.4221 | 05:57:29.94 +16:25:22.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 05 57 29.14 +16 25 49.5 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.3694+16.4221,2461128.6223,13.62,0.05,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
ATO J089.3694+16.4221 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:29.14 +16:25:49.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.54 05:57:55.44 +13:34:11.1
194.70752 -5.34728 galactic Ori Second-epoch detections are separated by 0.9" 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 | Gaia DR3 3343759274047207680 | 05:57:56.50 +13:33:49.9 (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 29.1223* 05 57 55.44 +13 34 11.1 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3343759274047207680,2461128.6223,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3343759274047207680 20260329.1223 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:55.44 +13:34:11.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.53 06:38:09.24 +15:02:40.6
198.03209 3.93190 galactic Gem Second-epoch detections are separated by 1.7" 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 | ATO J099.5395+15.0372 | 06:38:09.24 +15:02:40.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J099.5395+15.0372,2461128.6223,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.5395+15.0372 20260329.1223 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:38:09.24 +15:02:40.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.60 06:20:24.74 +14:14:42.3
196.75227 -0.24161 galactic Ori Second-epoch detections are separated by 0.7" 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 | 06:20:24.74 +14:14:42.3 (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 29.1223* 06 20 24.74 +14 14 42.3 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.60,0.05,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 20260329.1223 13.60CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:24.74 +14:14:42.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 52 33.54 +15 43 51.8 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348060808352992128,2461128.6223,13.77,0.05,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 3348060808352992128 20260329.1223 13.77CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:33.54 +15:43:51.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.62 06:06:40.77 +15:11:24.5
194.33261 -2.70511 galactic Ori Second-epoch detections are separated by 0.2" 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 | target | 06:06:40.77 +15:11:24.5 (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 29.1223* 06 06 40.77 +15 11 24.5 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.62,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:40.77 +15:11:24.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.71 06:13:23.70 +17:13:26.2
193.32889 -0.31169 galactic Ori Second-epoch detections are separated by 1.3" 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 | Gaia DR3 3370224798104166656 | 06:13:21.93 +17:13:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 13 23.70 +17 13 26.2 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3370224798104166656,2461128.6223,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3370224798104166656 20260329.1223 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:23.70 +17:13:26.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.60 05:51:05.92 +15:39:54.3
192.05554 -5.73302 galactic Tau Second-epoch detections are separated by 2.0" 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 | ATO J087.7798+15.6708 | 05:51:05.92 +15:39:54.3 (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 29.1223* 05 51 05.92 +15 39 54.3 13.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.7798+15.6708,2461128.6223,13.60,0.05,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 J087.7798+15.6708 20260329.1223 13.60CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:05.92 +15:39:54.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.53 06:00:36.43 +11:03:23.1
197.23139 -6.00969 galactic Ori Second-epoch detections are separated by 1.5" 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 | ATO J090.1521+11.0578 | 06:00:36.43 +11:03:23.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 00 36.43 +11 03 23.1 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.1521+11.0578,2461128.6223,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.1521+11.0578 20260329.1223 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:36.43 +11:03:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.47 06:21:53.66 +13:08:31.1
197.89497 -0.44337 galactic Ori Second-epoch detections are separated by 5.8" and 6.2 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 | ATO J095.4748+13.1397 | 06:21:53.96 +13:08:23.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 21 53.66 +13 08 31.1 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.4748+13.1397,2461128.6223,13.47,0.05,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
ATO J095.4748+13.1397 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:53.66 +13:08:31.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.46 06:26:36.79 +17:47:21.8
194.31679 2.73395 galactic Gem Second-epoch detections are separated by 1.7" 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 | ATO J096.6559+17.7948 | 06:26:36.41 +17:47:42.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.6559+17.7948,2461128.6223,13.46,0.05,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 J096.6559+17.7948 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:36.79 +17:47:21.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:09.43 +14:33:37.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 55 57.23 +16 32 15.4 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349620942333555840,2461128.6223,13.52,0.05,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
Gaia DR3 3349620942333555840 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:57.23 +16:32:15.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.31 05:56:51.70 +12:21:05.0
195.64422 -6.17363 galactic Ori 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 | Gaia DR3 3343064554498962432 | 05:56:49.89 +12:20:53.0 (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 29.1223* 05 56 51.70 +12 21 05.0 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3343064554498962432,2461128.6223,13.31,0.05,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 3343064554498962432 20260329.1223 13.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:51.70 +12:21:05.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 17 44.87 +14 40 48.6 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344917231590642048,2461128.6223,13.27,0.05,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 3344917231590642048 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:44.87 +14:40:48.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.27 06:21:40.48 +17:48:04.2
193.75716 1.69986 galactic Gem Second-epoch detections are separated by 1.2" 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 | ATO J095.4039+17.7981 | 06:21:38.76 +17:48:06.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5) J-Ks=0.320+/-0.179 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.4039+17.7981,2461128.6223,13.27,0.05,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
ATO J095.4039+17.7981 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:40.48 +17:48:04.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.13 05:48:32.31 +11:28:52.5
195.38601 -8.37284 galactic Ori Second-epoch detections are separated by 1.1" 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 | Gaia DR3 3337133548260370048 | 05:48:32.47 +11:29:08.9 (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 29.1223* 05 48 32.31 +11 28 52.5 13.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3337133548260370048,2461128.6223,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3337133548260370048 20260329.1223 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:32.31 +11:28:52.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 12.96 06:13:17.34 +11:55:02.2
197.97877 -2.87299 galactic Ori Second-epoch detections are separated by 5.0" and 5.5 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 3331898842118378368 | 06:13:15.80 +11:55:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8V 1959ApJS....4...23M LF 8 +11 5
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 29.1223* 06 13 17.34 +11 55 02.2 13.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3331898842118378368,2461128.6223,12.96,0.05,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 3331898842118378368 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:17.34 +11:55:02.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 12.95 06:11:10.67 +17:30:32.5
192.82471 -0.63873 galactic Ori Second-epoch detections are separated by 0.5" 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 | Large-amplitude variable Gaia DR2 3373230450575549696 | 06:11:09.63 +17:30:36.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 11 10.67 +17 30 32.5 12.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3373230450575549696,2461128.6223,12.95,0.05,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
Large-amplitude variable Gaia DR2 3373230450575549696 20260329.1223 12.95CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:10.67 +17:30:32.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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
EPIC 202093007,2461128.6223,12.89,0.05,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
EPIC 202093007 20260329.1223 12.89CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:25.39 +17:42:20.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 56 53.22 +14 50 24.1 12.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6223,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.1223 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:53.22 +14:50:24.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 12.86 06:03:45.62 +14:20:46.8
194.72641 -3.73243 galactic Ori 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 | 06:03:45.62 +14:20:46.8 (user input) | T | P | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.976+/-0.243 (M)
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 29.1223* 06 03 45.62 +14 20 46.8 12.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,12.86,0.05,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 20260329.1223 12.86CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:45.62 +14:20:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 16 27.35 +16 42 37.0 12.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3369945900107354240,2461128.6223,12.94,0.05,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
Gaia DR3 3369945900107354240 20260329.1223 12.94CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:27.35 +16:42:37.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.06 06:10:11.93 +17:42:34.7
192.53644 -0.74634 galactic Ori Second-epoch detections are separated by 0.6" 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 | ATO J092.5468+17.7042 | 06:10:11.93 +17:42:34.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 10 11.93 +17 42 34.7 13.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.5468+17.7042,2461128.6223,13.06,0.05,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
ATO J092.5468+17.7042 20260329.1223 13.06CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:11.93 +17:42:34.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 05 20.88 +15 10 13.7 12.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345577767498781824,2461128.6223,12.95,0.05,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
Gaia DR3 3345577767498781824 20260329.1223 12.95CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:20.88 +15:10:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 19 42.37 +15 59 26.5 13.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.08,0.05,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 20260329.1223 13.08CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:42.37 +15:59:26.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.31 05:57:13.85 +17:30:31.4
191.19427 -3.53743 galactic Ori Second-epoch detections are separated by 0.5" 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 | Gaia DR3 3349833182437442048 | 05:57:14.06 +17:31:03.9 (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 29.1223* 05 57 13.85 +17 30 31.4 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349833182437442048,2461128.6223,13.31,0.05,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 3349833182437442048 20260329.1223 13.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:13.85 +17:30:31.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 57 47.55 +14 19 56.9 13.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6223,13.23,0.05,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 20260329.1223 13.23CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:47.55 +14:19:56.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 3355237423827437568,2461128.6223,13.04,0.05,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 3355237423827437568 20260329.1223 13.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:06.81 +12:37:59.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.01 06:13:39.25 +12:47:36.1
197.25073 -2.37646 galactic Ori Second-epoch detections are separated by 7.4" and 6.2 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 | ATO J093.4071+12.8058 | 06:13:37.05 +12:48:04.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1IV (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 29.1223* 06 13 39.25 +12 47 36.1 13.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.4071+12.8058,2461128.6223,13.01,0.05,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 J093.4071+12.8058 20260329.1223 13.01CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:39.25 +12:47:36.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 17 11.07 +15 50 13.9 13.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3369820933739293184,2461128.6223,13.23,0.05,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 3369820933739293184 20260329.1223 13.23CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:11.07 +15:50:13.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.31 06:06:57.44 +18:07:52.5
191.79374 -1.21628 galactic Ori Second-epoch detections are separated by 1.9" 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 J091.7415+18.1453 | 06:06:56.83 +18:08:11.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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!
TCP 2026 03 29.1223* 06 06 57.44 +18 07 52.5 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.7415+18.1453,2461128.6223,13.31,0.05,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 J091.7415+18.1453 20260329.1223 13.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:57.44 +18:07:52.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.23 05:58:23.29 +14:59:59.7
193.51543 -4.54259 galactic Ori Second-epoch detections are separated by 0.6" 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 | ATO J089.5840+14.9921 | 05:58:21.46 +14:59:49.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1931AnHar.100...61C HD 249794
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 29.1223* 05 58 23.29 +14 59 59.7 13.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5840+14.9921,2461128.6223,13.23,0.05,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 J089.5840+14.9921 20260329.1223 13.23CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:23.29 +14:59:59.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.41 05:56:44.03 +17:00:10.6
191.57431 -3.89249 galactic Ori Second-epoch detections are separated by 0.7" 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 | ATO J089.1810+17.0131 | 05:56:44.38 +17:00:29.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 05 56 44.03 +17 00 10.6 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1810+17.0131,2461128.6223,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.1810+17.0131 20260329.1223 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:44.03 +17:00:10.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.28 06:22:11.59 +16:05:21.9
195.32709 1.00548 galactic Ori Second-epoch detections are separated by 0.5" 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 3369142569422792832 | 06:22:10.48 +16:05:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (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 29.1223* 06 22 11.59 +16 05 21.9 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3369142569422792832,2461128.6223,13.28,0.05,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 3369142569422792832 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:11.59 +16:05:21.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.31 06:10:30.86 +14:52:41.5
195.05412 -2.04562 galactic Ori Second-epoch detections are separated by 0.2" 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 3345637484724562688 | 06:10:29.56 +14:53:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5 1959ApJS....4...23M LF 8 +14 68 J-Ks=3.446+/- (Very red!)
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 29.1223* 06 10 30.86 +14 52 41.5 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345637484724562688,2461128.6223,13.31,0.05,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 3345637484724562688 20260329.1223 13.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:30.86 +14:52:41.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 09 52.24 +11 19 55.9 13.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EE Ori,2461128.6223,13.25,0.05,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
EE Ori 20260329.1223 13.25CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:52.24 +11:19:55.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.07 06:36:13.58 +13:05:53.3
199.55311 2.62751 galactic Gem Second-epoch detections are separated by 1.1" 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 | Gaia DR3 3355354899773041664 | 06:36:14.11 +13:06:16.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: em 1950ApJ...112...72M AS 131
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 3355354899773041664,2461128.6223,13.07,0.05,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 3355354899773041664 20260329.1223 13.07CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:13.58 +13:05:53.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 08 14.29 +13 57 07.0 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J060814.45+135710.5,2461128.6223,13.28,0.05,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
ZTF J060814.45+135710.5 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:14.29 +13:57:07.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.30 06:17:52.57 +15:42:08.5
195.17857 -0.09232 galactic Ori Second-epoch detections are separated by 0.9" 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 | ATO J094.4766+15.7123 | 06:17:52.57 +15:42:08.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 17 52.57 +15 42 08.5 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.4766+15.7123,2461128.6223,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.4766+15.7123 20260329.1223 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:52.57 +15:42:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.19 06:23:30.72 +15:36:13.9
195.90478 1.05790 galactic Ori Second-epoch detections are separated by 0.3" 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 | Gaia DR3 3368909777902231680 | 06:23:32.43 +15:35:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1959ApJS....4...23M LF 8 +15 270
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 29.1223* 06 23 30.72 +15 36 13.9 13.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3368909777902231680,2461128.6223,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368909777902231680 20260329.1223 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:30.72 +15:36:13.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.29 06:15:00.70 +14:58:53.8
195.48419 -1.04259 galactic Ori Second-epoch detections are separated by 1.1" 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 | Gaia DR3 3344984679757030528 | 06:15:01.62 +14:59:22.0 (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 29.1223* 06 15 00.70 +14 58 53.8 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344984679757030528,2461128.6223,13.29,0.05,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 3344984679757030528 20260329.1223 13.29CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:00.70 +14:58:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.40 06:00:20.50 +15:32:27.3
193.27716 -3.86570 galactic Ori Second-epoch detections are separated by 1.0" 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 J090.0761+15.5386 | 06:00:19.05 +15:32:43.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 00 20.50 +15 32 27.3 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.0761+15.5386,2461128.6223,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.0761+15.5386 20260329.1223 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:20.50 +15:32:27.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.43 06:18:18.07 +14:22:18.5
196.39891 -0.63245 galactic Ori Second-epoch detections are separated by 1.1" 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 | Gaia DR3 3344703621395907584 | 06:18:19.58 +14:22:27.5 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A0 1959ApJS....4...23M LF 8 +14 258
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 29.1223* 06 18 18.07 +14 22 18.5 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344703621395907584,2461128.6223,13.43,0.05,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 3344703621395907584 20260329.1223 13.43CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:18.07 +14:22:18.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.43 06:01:23.34 +13:54:28.3
194.82769 -4.44837 galactic Ori Second-epoch detections are separated by 1.3" and 5.5 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 3343843970803452928 | 06:01:23.30 +13:54:48.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (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 29.1223* 06 01 23.34 +13 54 28.3 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3343843970803452928,2461128.6223,13.43,0.05,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 3343843970803452928 20260329.1223 13.43CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:23.34 +13:54:28.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.44 06:14:42.27 +15:10:59.3
195.27167 -1.01159 galactic Ori Second-epoch detections are separated by 2.3" 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 | Gaia DR3 3345004097307291776 | 06:14:44.53 +15:10:59.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1959ApJS....4...23M LF 8 +15 116
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 29.1223* 06 14 42.27 +15 10 59.3 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345004097307291776,2461128.6223,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3345004097307291776 20260329.1223 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:42.27 +15:10:59.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.39 06:25:09.40 +15:58:53.2
195.75591 1.58417 galactic Ori Second-epoch detections are separated by 1.3" 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 | Gaia DR3 3368959152842877696 | 06:25:07.99 +15:59:10.9 (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 29.1223* 06 25 09.40 +15 58 53.2 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3368959152842877696,2461128.6223,13.39,0.05,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 3368959152842877696 20260329.1223 13.39CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:09.40 +15:58:53.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 12 57.12 +17 26 20.8 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J061257.09+172613.7,2461128.6223,13.46,0.05,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
ZTF J061257.09+172613.7 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:57.12 +17:26:20.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.54 05:59:57.47 +13:03:23.9
195.40066 -5.16924 galactic Ori Second-epoch detections are separated by 0.3" and 5.5 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 | ATO J089.9895+13.0544 | 05:59:57.47 +13:03:23.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 59 57.47 +13 03 23.9 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.9895+13.0544,2461128.6223,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.9895+13.0544 20260329.1223 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:57.47 +13:03:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 14 37.19 +16 02 30.0 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.43,0.05,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 20260329.1223 13.43CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:37.19 +16:02:30.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.46 06:26:56.70 +16:47:33.6
195.23728 2.34139 galactic Gem Second-epoch detections are separated by 1.4" 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 | Gaia DR3 3369575635270175104 | 06:26:55.35 +16:48:01.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 3369575635270175104,2461128.6223,13.46,0.05,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 3369575635270175104 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:56.70 +16:47:33.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 07 01.07 +10 58 45.7 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3330233872279561984,2461128.6223,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3330233872279561984 20260329.1223 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:01.07 +10:58:45.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.42 06:22:17.55 +14:40:26.2
196.58808 0.36182 galactic Ori Second-epoch detections are separated by 3.8" 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 3368700217854970624 | 06:22:18.91 +14:40:41.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1959ApJS....4...23M LF 8 +14 333
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 29.1223* 06 22 17.55 +14 40 26.2 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3368700217854970624,2461128.6223,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368700217854970624 20260329.1223 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:17.55 +14:40:26.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.53 05:53:52.19 +10:13:57.5
197.13721 -7.85631 galactic Ori Second-epoch detections are separated by 1.7" 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 | Gaia DR3 3335987002446976768 | 05:53:52.25 +10:14:35.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1931AnHar.100...61C HD 248978
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 29.1223* 05 53 52.19 +10 13 57.5 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3335987002446976768,2461128.6223,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3335987002446976768 20260329.1223 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:52.19 +10:13:57.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.56 05:49:29.16 +13:54:40.7
193.38222 -6.95333 galactic Tau Second-epoch detections are separated by 0.9" 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 J087.3719+13.9120 | 05:49:29.16 +13:54:40.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 49 29.16 +13 54 40.7 13.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.3719+13.9120,2461128.6223,13.56,0.05,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
ATO J087.3719+13.9120 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:29.16 +13:54:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 12 28.12 +15 20 04.0 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:28.12 +15:20:04.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.46 06:11:37.12 +15:28:25.8
194.65996 -1.52545 galactic Ori Second-epoch detections are separated by 1.2" 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 | Gaia DR3 3345733966869577344 | 06:11:39.14 +15:28:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1959ApJS....4...23M LF 8 +15 49
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 29.1223* 06 11 37.12 +15 28 25.8 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345733966869577344,2461128.6223,13.46,0.05,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 3345733966869577344 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:37.12 +15:28:25.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.60 05:52:38.40 +15:49:35.6
192.10289 -5.33127 galactic Tau Second-epoch detections are separated by 1.2" and 5.6 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 | ASASSN-V J055236.39+154932.7 | 05:52:36.38 +15:49:34.0 (Gaia DR3) | ROT: (local) | d (local) | Gaia3var=NOT_AVAILABLE SpType: A0 1958PMcCO..13b....V TYC 1312-2581-1
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 29.1223* 05 52 38.40 +15 49 35.6 13.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055236.39+154932.7,2461128.6223,13.60,0.05,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
ASASSN-V J055236.39+154932.7 20260329.1223 13.60CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:38.40 +15:49:35.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.66 06:12:18.14 +15:12:21.6
194.97416 -1.50951 galactic Ori Second-epoch detections are separated by 0.7" 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 J093.0787+15.2153 | 06:12:16.28 +15:12:50.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8V 1959ApJS....4...23M LF 8 +15 60
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 29.1223* 06 12 18.14 +15 12 21.6 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.0787+15.2153,2461128.6223,13.66,0.05,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 J093.0787+15.2153 20260329.1223 13.66CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:18.14 +15:12:21.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 58 27.75 +14 56 55.0 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:27.75 +14:56:55.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.38 06:34:47.10 +15:31:02.4
197.23919 3.42448 galactic Gem Second-epoch detections are separated by 2.4" and 5.5 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 3357086385767980544 | 06:34:47.11 +15:31:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 3357086385767980544,2461128.6223,13.38,0.05,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
Gaia DR3 3357086385767980544 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:47.10 +15:31:02.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.37 06:00:02.61 +11:09:52.3
197.06864 -6.07761 galactic Ori Second-epoch detections are separated by 1.0" 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 | Gaia DR3 3342119764771209472 | 06:00:05.46 +11:09:58.8 (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 29.1223* 06 00 02.61 +11 09 52.3 13.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3342119764771209472,2461128.6223,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3342119764771209472 20260329.1223 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:02.61 +11:09:52.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.50 06:00:51.40 +10:59:28.2
197.31869 -5.98805 galactic Ori Second-epoch detections are separated by 0.3" 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 | Gaia DR3 3341914435273738624 | 06:00:53.25 +10:59:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1931AnHar.100...61C HD 250362
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 29.1223* 06 00 51.40 +10 59 28.2 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3341914435273738624,2461128.6223,13.50,0.05,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
Gaia DR3 3341914435273738624 20260329.1223 13.50CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:51.40 +10:59:28.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.57 06:19:47.12 +16:38:52.2
194.56243 0.75882 galactic Ori Second-epoch detections are separated by 1.5" 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 J094.9454+16.6480 | 06:19:46.82 +16:39:33.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 19 47.12 +16 38 52.2 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.9454+16.6480,2461128.6223,13.57,0.05,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
ATO J094.9454+16.6480 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:47.12 +16:38:52.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.74 05:52:46.77 +15:24:02.9
192.48967 -5.51600 galactic Tau Second-epoch detections are separated by 1.2" and 5.5 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 | ATO J088.1971+15.4055 | 05:52:46.77 +15:24:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1223* 05 52 46.77 +15 24 02.9 13.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.1971+15.4055,2461128.6223,13.74,0.05,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
ATO J088.1971+15.4055 20260329.1223 13.74CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:46.77 +15:24:02.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.62 06:11:09.03 +17:31:03.4
192.81404 -0.64030 galactic Ori Second-epoch detections are separated by 0.5" 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 | Large-amplitude variable Gaia DR2 3373230450575549696 | 06:11:09.63 +17:30:36.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 11 09.03 +17 31 03.4 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3373230450575549696,2461128.6223,13.62,0.05,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
Large-amplitude variable Gaia DR2 3373230450575549696 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:09.03 +17:31:03.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.62 06:17:01.32 +18:06:38.1
192.96171 0.87058 galactic Ori Second-epoch detections are separated by 3.0" 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 | 06:17:01.32 +18:06:38.1 (user input) | T | P | (position from user input) SpType: F3 (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 29.1223* 06 17 01.32 +18 06 38.1 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.62,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:01.32 +18:06:38.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 12 21.10 +15 28 31.8 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J061222.54+152832.9,2461128.6223,13.50,0.05,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
ZTF J061222.54+152832.9 20260329.1223 13.50CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:21.10 +15:28:31.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.44 06:27:16.30 +15:59:50.2
195.97862 2.04140 galactic Gem Second-epoch detections are separated by 0.4" 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 | Gaia DR3 3369275060578136704 | 06:27:15.70 +15:59:14.9 (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 3369275060578136704,2461128.6223,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3369275060578136704 20260329.1223 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:16.30 +15:59:50.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.54 06:16:19.71 +14:31:17.4
196.04048 -0.98178 galactic Ori 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 | Gaia DR3 3344815324905336320 | 06:16:21.97 +14:31:07.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0V 1959ApJS....4...23M LF 8 +14 215
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 29.1223* 06 16 19.71 +14 31 17.4 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344815324905336320,2461128.6223,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3344815324905336320 20260329.1223 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:19.71 +14:31:17.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.52 06:21:47.10 +17:02:50.5
194.43525 1.36905 galactic Ori Second-epoch detections are separated by 1.2" 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 | Gaia DR3 3370011458488899200 | 06:21:46.79 +17:03:13.8 (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 29.1223* 06 21 47.10 +17 02 50.5 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3370011458488899200,2461128.6223,13.52,0.05,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
Gaia DR3 3370011458488899200 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:47.10 +17:02:50.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.69 05:50:50.22 +14:25:30.8
193.10090 -6.41177 galactic Tau Second-epoch detections are separated by 3.5" 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 | 05:50:50.22 +14:25:30.8 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 50 50.22 +14 25 30.8 13.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.69,0.05,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 20260329.1223 13.69CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:50.22 +14:25:30.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.60 06:13:44.01 +14:52:17.4
195.43345 -1.36644 galactic Ori Second-epoch detections are separated by 1.8" 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 J093.4373+14.8701 | 06:13:43.06 +14:51:40.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 1959ApJS....4...23M LF 8 +14 143
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 29.1223* 06 13 44.01 +14 52 17.4 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.4373+14.8701,2461128.6223,13.60,0.05,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 J093.4373+14.8701 20260329.1223 13.60CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:44.01 +14:52:17.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.71 05:57:13.85 +17:08:13.1
191.51721 -3.72271 galactic Ori Second-epoch detections are separated by 3.8" 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 | 05:57:13.85 +17:08:13.1 (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 29.1223* 05 57 13.85 +17 08 13.1 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:13.85 +17:08:13.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.52 06:15:27.96 +14:23:53.8
196.04947 -1.22406 galactic Ori Second-epoch detections are separated by 0.1" 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 3344809827347251968 | 06:15:30.14 +14:23:37.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1959ApJS....4...23M LF 8 +14 190
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 29.1223* 06 15 27.96 +14 23 53.8 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344809827347251968,2461128.6223,13.52,0.05,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
Gaia DR3 3344809827347251968 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:27.96 +14:23:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.87 05:52:19.39 +15:41:14.0
192.18540 -5.46720 galactic Tau Second-epoch detections are separated by 1.7" 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 | ATO J088.0824+15.6788 | 05:52:19.39 +15:41:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 52 19.39 +15 41 14.0 13.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.0824+15.6788,2461128.6223,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.0824+15.6788 20260329.1223 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:19.39 +15:41:14.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 19 12.08 +12 45 05.6 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3332386995222063616,2461128.6223,13.55,0.05,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 3332386995222063616 20260329.1223 13.55CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:12.08 +12:45:05.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.57 06:06:58.48 +14:36:07.6
194.88197 -2.92825 galactic Ori Second-epoch detections are separated by 1.6" 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 J091.7404+14.6020 | 06:06:58.48 +14:36:07.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 06 58.48 +14 36 07.6 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.7404+14.6020,2461128.6223,13.57,0.05,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
ATO J091.7404+14.6020 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:58.48 +14:36:07.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.69 06:18:12.86 +17:18:43.0
193.79958 0.74184 galactic Ori Second-epoch detections are separated by 0.7" 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 | ATO J094.5676+17.3141 | 06:18:15.37 +17:18:22.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K1 (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 29.1223* 06 18 12.86 +17 18 43.0 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.5676+17.3141,2461128.6223,13.69,0.05,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 J094.5676+17.3141 20260329.1223 13.69CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:12.86 +17:18:43.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.65 06:27:44.20 +17:39:44.9
194.55355 2.91218 galactic Gem Second-epoch detections are separated by 1.7" 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 | ATO J096.9262+17.6679 | 06:27:43.94 +17:40:16.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.9262+17.6679,2461128.6223,13.65,0.05,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 J096.9262+17.6679 20260329.1223 13.65CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:44.20 +17:39:44.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.62 06:14:33.77 +14:45:32.8
195.62800 -1.24407 galactic Ori Second-epoch detections are separated by 1.0" 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 J093.6382+14.7567 | 06:14:35.31 +14:45:23.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9 1959ApJS....4...23M LF 8 +14 170
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 29.1223* 06 14 33.77 +14 45 32.8 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.6382+14.7567,2461128.6223,13.62,0.05,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
ATO J093.6382+14.7567 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:33.77 +14:45:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 03 52.31 +14 59 06.2 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345547457913147008,2461128.6223,13.70,0.05,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 3345547457913147008 20260329.1223 13.70CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:52.31 +14:59:06.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.55 06:27:05.36 +15:18:40.6
196.56597 1.68376 galactic Gem Second-epoch detections are separated by 1.6" 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 | ATO J096.7740+15.2999 | 06:27:06.07 +15:18:12.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.7740+15.2999,2461128.6223,13.55,0.05,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 J096.7740+15.2999 20260329.1223 13.55CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:05.36 +15:18:40.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.59 06:25:36.83 +14:06:33.7
197.46355 0.80818 galactic Gem Second-epoch detections are separated by 1.2" 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 | ATO J096.4007+14.1045 | 06:25:36.83 +14:06:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J096.4007+14.1045,2461128.6223,13.59,0.05,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
ATO J096.4007+14.1045 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:36.83 +14:06:33.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.77 05:59:07.20 +15:23:10.3
193.26633 -4.19807 galactic Ori Second-epoch detections are separated by 3.4" 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 | ATO J089.7943+15.3982 | 05:59:08.93 +15:23:37.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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!
TCP 2026 03 29.1223* 05 59 07.20 +15 23 10.3 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.7943+15.3982,2461128.6223,13.77,0.05,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 J089.7943+15.3982 20260329.1223 13.77CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:07.20 +15:23:10.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.65 06:12:31.19 +15:20:14.8
194.88396 -1.40042 galactic Ori Second-epoch detections are separated by 5.4" 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 J093.1411+15.3416 | 06:12:31.19 +15:20:14.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 12 31.19 +15 20 14.8 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.1411+15.3416,2461128.6223,13.65,0.05,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 J093.1411+15.3416 20260329.1223 13.65CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:31.19 +15:20:14.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.80 06:12:58.78 +16:22:06.4
194.03213 -0.80895 galactic Ori Second-epoch detections are separated by 1.9" 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 3346083916508271232 | 06:13:00.98 +16:21:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 12 58.78 +16 22 06.4 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3346083916508271232,2461128.6223,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3346083916508271232 20260329.1223 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:58.78 +16:22:06.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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
ZTF J062600.88+163945.8,2461128.6223,13.66,0.05,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
ZTF J062600.88+163945.8 20260329.1223 13.66CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:01.08 +16:39:51.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.72 06:17:50.72 +16:23:57.8
194.56135 0.23164 galactic Ori Second-epoch detections are separated by 1.7" 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 J094.4582+16.3982 | 06:17:51.61 +16:23:29.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 17 50.72 +16 23 57.8 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.4582+16.3982,2461128.6223,13.72,0.05,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
ATO J094.4582+16.3982 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:50.72 +16:23:57.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.61 05:58:48.36 +13:38:12.1
194.75521 -5.12783 galactic Ori Second-epoch detections are separated by 0.6" 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 | Gaia DR3 3343853149152246784 | 05:58:50.69 +13:38:09.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 58 48.36 +13 38 12.1 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3343853149152246784,2461128.6223,13.61,0.05,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 3343853149152246784 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:48.36 +13:38:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 14 14.15 +13 14 59.7 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344122044166361984,2461128.6223,13.76,0.05,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 3344122044166361984 20260329.1223 13.76CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:14.15 +13:14:59.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.85 05:48:08.74 +15:56:46.3
191.45032 -6.20341 galactic Tau Second-epoch detections are separated by 2.6" 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 | 05:48:08.74 +15:56:46.3 (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 29.1223* 05 48 08.74 +15 56 46.3 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.85,0.05,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 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:08.74 +15:56:46.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 54 30.48 +12 57 31.2 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.69,0.05,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 20260329.1223 13.69CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:30.48 +12:57:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.79 05:57:54.95 +15:49:12.1
192.74442 -4.23507 galactic Ori Second-epoch detections are separated by 0.7" 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 | 05:57:54.95 +15:49:12.1 (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 29.1223* 05 57 54.95 +15 49 12.1 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.79,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:54.95 +15:49:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.63 06:18:54.39 +11:33:58.2
198.94130 -1.82945 galactic Ori Second-epoch detections are separated by 1.2" 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 J094.7333+11.5622 | 06:18:55.98 +11:33:56.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 18 54.39 +11 33 58.2 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.7333+11.5622,2461128.6223,13.63,0.05,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
ATO J094.7333+11.5622 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:54.39 +11:33:58.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.53 06:03:20.61 +10:39:27.7
197.90996 -5.61649 galactic Ori Second-epoch detections are separated by 2.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.8250+10.6657 | 06:03:18.10 +10:39:21.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 03 20.61 +10 39 27.7 13.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.8250+10.6657,2461128.6223,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.8250+10.6657 20260329.1223 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:20.61 +10:39:27.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.70 06:00:57.41 +16:27:52.0
192.54525 -3.28162 galactic Ori Second-epoch detections are separated by 1.4" 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 | Gaia DR3 3348915644282911488 | 06:00:55.41 +16:28:05.7 (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!
TCP 2026 03 29.1223* 06 00 57.41 +16 27 52.0 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348915644282911488,2461128.6223,13.70,0.05,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 3348915644282911488 20260329.1223 13.70CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:57.41 +16:27:52.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.83 05:56:21.71 +17:58:16.1
190.68936 -3.48584 galactic Ori Second-epoch detections are separated by 3.2" 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 | Gaia DR3 3350422147011829760 | 05:56:22.34 +17:58:44.4 (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 29.1223* 05 56 21.71 +17 58 16.1 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3350422147011829760,2461128.6223,13.83,0.05,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
Gaia DR3 3350422147011829760 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:21.71 +17:58:16.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.73 05:56:34.56 +10:29:34.4
197.23863 -7.14883 galactic Ori Second-epoch detections are separated by 0.9" 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 | Gaia DR3 3341973602742733696 | 05:56:35.53 +10:30:05.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1931AnHar.100...61C HD 249492
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 29.1223* 05 56 34.56 +10 29 34.4 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3341973602742733696,2461128.6223,13.73,0.05,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
Gaia DR3 3341973602742733696 20260329.1223 13.73CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:34.56 +10:29:34.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.62 06:33:00.95 +16:03:44.3
196.55863 3.29580 galactic Gem Second-epoch detections are separated by 0.5" 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 | ATO J098.2516+16.0672 | 06:33:00.95 +16:03:44.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J098.2516+16.0672,2461128.6223,13.62,0.05,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
ATO J098.2516+16.0672 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:33:00.95 +16:03:44.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 51 00.51 +13 29 08.8 13.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3346439269219001472,2461128.6223,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3346439269219001472 20260329.1223 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:00.51 +13:29:08.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 02 23.83 +16 35 57.0 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.91,0.05,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
target 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:23.83 +16:35:57.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.71 06:11:05.92 +16:19:10.0
193.85826 -1.22824 galactic Ori Second-epoch detections are separated by 3.3" 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 | EG Ori | 06:11:07.11 +16:19:34.1 (Gaia DR3) | EA/SD (local) | 1.163166000000 (local) | Gaia3var=VARIABLE SpType: G0V 1984PASP...96...98H EG Ori
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 29.1223* 06 11 05.92 +16 19 10.0 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EG Ori,2461128.6223,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EG Ori 20260329.1223 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:05.92 +16:19:10.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.94 05:55:47.19 +14:48:03.3
193.37582 -5.18704 galactic Ori Second-epoch detections are separated by 3.4" 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 | ATO J088.9441+14.8079 | 05:55:47.19 +14:48:03.3 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 55 47.19 +14 48 03.3 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.9441+14.8079,2461128.6223,13.94,0.05,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
ATO J088.9441+14.8079 20260329.1223 13.94CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:47.19 +14:48:03.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 13 31.18 +17 23 07.5 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J061331.20+172301.2,2461128.6223,13.82,0.05,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
ZTF J061331.20+172301.2 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:31.18 +17:23:07.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.89 05:57:00.08 +17:55:39.2
190.80330 -3.37586 galactic Ori Second-epoch detections are separated by 0.4" 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 | target | 05:57:00.08 +17:55:39.2 (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 29.1223* 05 57 00.08 +17 55 39.2 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.89,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:00.08 +17:55:39.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 09 55.61 +14 26 05.8 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.82,0.05,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
target 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:55.61 +14:26:05.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 14 08.40 +17 22 59.2 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.77,0.05,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 20260329.1223 13.77CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:08.40 +17:22:59.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 55 13.00 +12 41 16.7 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:13.00 +12:41:16.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 20 58.44 +14 41 23.0 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062058.41+144114.8,2461128.6223,13.73,0.05,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
ASASSN-V J062058.41+144114.8 20260329.1223 13.73CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:58.44 +14:41:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.64 06:20:57.41 +16:50:14.0
194.52760 1.09544 galactic Ori 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 | ATO J095.2326+16.8424 | 06:20:57.44 +16:50:41.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 20 57.41 +16 50 14.0 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.2326+16.8424,2461128.6223,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.2326+16.8424 20260329.1223 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:57.41 +16:50:14.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 3369382602261570688,2461128.6223,13.66,0.05,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 3369382602261570688 20260329.1223 13.66CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:51.97 +16:41:06.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 19 32.57 +13 26 12.2 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.68,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:32.57 +13:26:12.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.76 05:53:13.24 +14:40:26.3
193.17539 -5.78800 galactic Ori Second-epoch detections are separated by 1.4" 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 | Gaia DR3 3347084712605690112 | 05:53:11.07 +14:40:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (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 29.1223* 05 53 13.24 +14 40 26.3 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3347084712605690112,2461128.6223,13.76,0.05,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 3347084712605690112 20260329.1223 13.76CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:13.24 +14:40:26.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 14 22.25 +10 07 40.1 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.65,0.05,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 20260329.1223 13.65CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:22.25 +10:07:40.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 49 14.22 +14 41 49.9 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3347873341620021248,2461128.6223,13.81,0.05,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
Gaia DR3 3347873341620021248 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:14.22 +14:41:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 50 03.76 +10 24 30.6 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3336673681818468096,2461128.6223,13.72,0.05,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
Gaia DR3 3336673681818468096 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:03.76 +10:24:30.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.69 06:12:26.70 +15:00:24.6
195.16550 -1.57485 galactic Ori Second-epoch detections are separated by 1.4" 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 | ATO J093.1120+15.0101 | 06:12:26.70 +15:00:24.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 12 26.70 +15 00 24.6 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.1120+15.0101,2461128.6223,13.69,0.05,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 J093.1120+15.0101 20260329.1223 13.69CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:26.70 +15:00:24.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.81 06:01:37.68 +14:43:11.4
194.14676 -3.99948 galactic Ori Second-epoch detections are separated by 1.7" 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 | Gaia DR3 3345434448731575424 | 06:01:35.74 +14:43:33.3 (Gaia DR3) | T | P | 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 29.1223* 06 01 37.68 +14 43 11.4 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345434448731575424,2461128.6223,13.81,0.05,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
Gaia DR3 3345434448731575424 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:37.68 +14:43:11.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 14 35.97 +13 49 52.3 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:35.97 +13:49:52.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.01 06:06:48.48 +16:40:37.7
193.04715 -1.95513 galactic Ori Second-epoch detections are separated by 0.3" 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 J091.7202+16.6787 | 06:06:51.00 +16:40:41.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.798+/-0.124 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 06 48.48 +16 40 37.7 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.7202+16.6787,2461128.6223,14.01,0.05,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 J091.7202+16.6787 20260329.1223 14.01CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:48.48 +16:40:37.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.03 06:05:37.22 +17:10:44.5
192.47013 -1.95859 galactic Ori 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 | ATO J091.4017+17.1781 | 06:05:37.22 +17:10:44.5 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1223* 06 05 37.22 +17 10 44.5 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.4017+17.1781,2461128.6223,14.03,0.05,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
ATO J091.4017+17.1781 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:37.22 +17:10:44.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.74 06:18:28.69 +14:20:27.4
196.44639 -0.60930 galactic Ori Second-epoch detections are separated by 5.1" and 6.0 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 | 06:18:28.69 +14:20:27.4 (user input) | T | P | (position from user input) SpType: A7V (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 29.1223* 06 18 28.69 +14 20 27.4 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.74,0.05,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
target 20260329.1223 13.74CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:28.69 +14:20:27.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.95 06:08:55.81 +17:07:39.8
192.89953 -1.29261 galactic Ori Second-epoch detections are separated by 2.4" and 5.5 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 | ATO J092.2210+17.1268 | 06:08:53.04 +17:07:36.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 08 55.81 +17 07 39.8 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.2210+17.1268,2461128.6223,13.95,0.05,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
ATO J092.2210+17.1268 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:55.81 +17:07:39.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.87 05:55:56.50 +14:38:13.7
193.53723 -5.23595 galactic Ori Second-epoch detections are separated by 2.3" and 5.8 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 3346978682752384256 | 05:55:56.20 +14:38:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 55 56.50 +14 38 13.7 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3346978682752384256,2461128.6223,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3346978682752384256 20260329.1223 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:56.50 +14:38:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 17 35.47 +14 21 38.3 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.83,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:35.47 +14:21:38.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.94 05:49:16.39 +11:26:25.1
195.51277 -8.23739 galactic Ori Second-epoch detections are separated by 3.6" 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 | ASASSN-V J054916.53+112547.2 | 05:49:16.53 +11:25:47.2 (Gaia DR3) | SR (local) | 2458559.68600 (local) | Gaia3var=NOT_AVAILABLE SpType: M3 (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 29.1223* 05 49 16.39 +11 26 25.1 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054916.53+112547.2,2461128.6223,13.94,0.05,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
ASASSN-V J054916.53+112547.2 20260329.1223 13.94CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:16.39 +11:26:25.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 15 10.86 +14 43 50.2 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.85,0.05,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 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:10.86 +14:43:50.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.77 06:18:34.84 +14:20:07.9
196.46292 -0.59000 galactic Ori Second-epoch detections are separated by 3.3" and 5.5 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 | ATO J094.6427+14.3345 | 06:18:34.84 +14:20:07.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 18 34.84 +14 20 07.9 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.6427+14.3345,2461128.6223,13.77,0.05,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 J094.6427+14.3345 20260329.1223 13.77CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:34.84 +14:20:07.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.87 06:09:57.09 +16:59:12.5
193.14097 -1.14710 galactic Ori 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 | Gaia DR3 3349191724779336448 | 06:09:54.61 +16:59:02.5 (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!
TCP 2026 03 29.1223* 06 09 57.09 +16 59 12.5 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349191724779336448,2461128.6223,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3349191724779336448 20260329.1223 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:57.09 +16:59:12.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.85 05:58:48.37 +16:29:35.8
192.26471 -3.71550 galactic Ori Second-epoch detections are separated by 1.1" 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 | ATO J089.7017+16.4915 | 05:58:48.37 +16:29:35.8 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 58 48.37 +16 29 35.8 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.7017+16.4915,2461128.6223,13.85,0.05,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 J089.7017+16.4915 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:48.37 +16:29:35.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.80 06:36:15.89 +17:59:27.2
195.19320 4.86670 galactic Gem Second-epoch detections are separated by 2.2" 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 | 06:36:15.89 +17:59:27.2 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:15.89 +17:59:27.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.81 06:10:46.63 +14:47:20.1
195.16302 -2.03293 galactic Ori Second-epoch detections are separated by 3.4" and 5.9 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 | ATO J092.6913+14.7916 | 06:10:46.63 +14:47:20.1 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1223* 06 10 46.63 +14 47 20.1 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.6913+14.7916,2461128.6223,13.81,0.05,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
ATO J092.6913+14.7916 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:46.63 +14:47:20.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.88 05:57:33.70 +15:38:37.6
192.85544 -4.39654 galactic Ori Second-epoch detections are separated by 0.9" 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 | ATO J089.3854+15.6467 | 05:57:32.76 +15:39:02.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2IV (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 29.1223* 05 57 33.70 +15 38 37.6 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.3854+15.6467,2461128.6223,13.88,0.05,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 J089.3854+15.6467 20260329.1223 13.88CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:33.70 +15:38:37.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 00 21.97 +10 05 26.5 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6223,13.83,0.05,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
VARIABLE_NAME 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:21.97 +10:05:26.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.74 06:02:09.43 +13:56:17.9
194.89268 -4.27097 galactic Ori Second-epoch detections are separated by 0.7" 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 | ASASSN-V J060207.36+135631.6 | 06:02:07.36 +13:56:31.6 (Gaia DR3) | SR (local) | 2459470.90500 (local) | 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 29.1223* 06 02 09.43 +13 56 17.9 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060207.36+135631.6,2461128.6223,13.74,0.05,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
ASASSN-V J060207.36+135631.6 20260329.1223 13.74CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:09.43 +13:56:17.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.94 06:00:57.68 +14:31:57.1
194.23090 -4.23196 galactic Ori Second-epoch detections are separated by 3.8" 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 | Gaia DR3 3345425244620411392 | 06:00:56.30 +14:32:12.9 (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 29.1223* 06 00 57.68 +14 31 57.1 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345425244620411392,2461128.6223,13.94,0.05,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
Gaia DR3 3345425244620411392 20260329.1223 13.94CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:57.68 +14:31:57.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 20 46.73 +15 42 08.3 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.79,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:46.73 +15:42:08.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.96 06:06:05.15 +13:21:02.3
195.87338 -3.72394 galactic Ori Second-epoch detections are separated by 1.0" 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 | Gaia DR3 3344300336848200576 | 06:06:06.68 +13:20:48.7 (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!
TCP 2026 03 29.1223* 06 06 05.15 +13 21 02.3 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344300336848200576,2461128.6223,13.96,0.05,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 3344300336848200576 20260329.1223 13.96CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:05.15 +13:21:02.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 23 30.13 +11 14 21.5 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3330874204660960768,2461128.6223,13.73,0.05,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
Gaia DR3 3330874204660960768 20260329.1223 13.73CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:30.13 +11:14:21.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.85 05:58:26.36 +15:59:27.8
192.65812 -4.04095 galactic Ori Second-epoch detections are separated by 0.4" 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 | Gaia DR3 3348824934574492416 | 05:58:26.25 +16:00:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1931AnHar.100...61C HD 249793
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 29.1223* 05 58 26.36 +15 59 27.8 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348824934574492416,2461128.6223,13.85,0.05,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 3348824934574492416 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:26.36 +15:59:27.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.96 06:15:37.99 +17:53:12.9
193.00139 0.47372 galactic Ori Second-epoch detections are separated by 2.5" 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 | Gaia DR3 3370369349523493248 | 06:15:35.83 +17:53:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 15 37.99 +17 53 12.9 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3370369349523493248,2461128.6223,13.96,0.05,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 3370369349523493248 20260329.1223 13.96CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:37.99 +17:53:12.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 17 24.85 +10 19 34.6 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3329253623300708608,2461128.6223,13.88,0.05,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 3329253623300708608 20260329.1223 13.88CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:24.85 +10:19:34.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.97 05:58:07.30 +16:38:48.8
192.04949 -3.78166 galactic Ori Second-epoch detections are separated by 4.7" and 5.8 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 | Brh V67 | 05:58:05.12 +16:39:01.5 (Gaia DR3) | S (local) | (local) | 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 29.1223* 05 58 07.30 +16 38 48.8 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Brh V67,2461128.6223,13.97,0.05,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
Brh V67 20260329.1223 13.97CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:07.30 +16:38:48.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.87 05:48:53.13 +10:13:09.1
196.53544 -8.92849 galactic Ori Second-epoch detections are separated by 1.8" 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 | 05:48:53.13 +10:13:09.1 (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 29.1223* 05 48 53.13 +10 13 09.1 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.13 +10:13:09.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.86 06:10:25.45 +13:28:04.0
196.28102 -2.74356 galactic Ori Second-epoch detections are separated by 1.8" 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 | 06:10:25.45 +13:28:04.0 (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 29.1223* 06 10 25.45 +13 28 04.0 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.86,0.05,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 20260329.1223 13.86CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:25.45 +13:28:04.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.79 05:49:28.19 +11:30:41.1
195.47483 -8.16014 galactic Ori Second-epoch detections are separated by 1.9" and 5.6 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 3337087682306216192 | 05:49:25.65 +11:30:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1931AnHar.100...61C HD 248081
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 29.1223* 05 49 28.19 +11 30 41.1 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3337087682306216192,2461128.6223,13.79,0.05,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
Gaia DR3 3337087682306216192 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:28.19 +11:30:41.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.78 06:05:57.84 +11:37:35.4
197.37134 -4.58502 galactic Ori Second-epoch detections are separated by 1.1" 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 | 06:05:57.84 +11:37:35.4 (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 29.1223* 06 05 57.84 +11 37 35.4 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,13.78,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:57.84 +11:37:35.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.89 06:19:04.36 +16:47:19.7
194.35756 0.67502 galactic Ori Second-epoch detections are separated by 1.8" 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 | ATO J094.7664+16.8094 | 06:19:04.07 +16:47:59.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.576+/-0.243 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 19 04.36 +16 47 19.7 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.7664+16.8094,2461128.6223,13.89,0.05,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
ATO J094.7664+16.8094 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:04.36 +16:47:19.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.98 06:16:58.67 +18:09:12.6
192.91896 0.88173 galactic Ori Second-epoch detections are separated by 1.9" 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 | ATO J094.2473+18.1622 | 06:17:00.89 +18:09:14.9 (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 29.1223* 06 16 58.67 +18 09 12.6 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.2473+18.1622,2461128.6223,13.98,0.05,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 J094.2473+18.1622 20260329.1223 13.98CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:58.67 +18:09:12.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 11 38.99 +15 16 52.1 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:38.99 +15:16:52.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.95 06:04:28.03 +16:29:14.2
192.93920 -2.53736 galactic Ori Second-epoch detections are separated by 0.7" 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 | ATO J091.1205+16.4924 | 06:04:28.94 +16:29:32.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 04 28.03 +16 29 14.2 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.1205+16.4924,2461128.6223,13.95,0.05,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
ATO J091.1205+16.4924 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:28.03 +16:29:14.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 21 31.34 +14 40 25.4 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.01,0.05,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 20260329.1223 14.01CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:31.34 +14:40:25.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.81 06:00:15.39 +12:08:18.0
196.24043 -5.55594 galactic Ori 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 | ATO J090.0652+12.1457 | 06:00:15.39 +12:08:18.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) 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 29.1223* 06 00 15.39 +12 08 18.0 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.0652+12.1457,2461128.6223,13.81,0.05,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
ATO J090.0652+12.1457 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:15.39 +12:08:18.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.96 05:57:29.86 +16:51:07.0
191.79675 -3.80932 galactic Ori Second-epoch detections are separated by 3.4" 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 | ASASSN-V J055728.15+165125.1 | 05:57:28.15 +16:51:25.1 (Gaia DR3) | SR (local) | 41.230000000000 (local) | Gaia3var=VARIABLE
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 29.1223* 05 57 29.86 +16 51 07.0 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055728.15+165125.1,2461128.6223,13.96,0.05,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
ASASSN-V J055728.15+165125.1 20260329.1223 13.96CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:29.86 +16:51:07.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 17 27.80 +11 05 42.3 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6223,13.91,0.05,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
VARIABLE_NAME 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:27.80 +11:05:42.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.19 06:06:00.97 +16:53:36.4
192.76576 -2.01532 galactic Ori Second-epoch detections are separated by 0.5" 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 | Gaia DR3 3349222408025645184 | 06:06:01.87 +16:54:01.8 (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 29.1223* 06 06 00.97 +16 53 36.4 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349222408025645184,2461128.6223,14.19,0.05,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
Gaia DR3 3349222408025645184 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:00.97 +16:53:36.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.04 06:25:33.68 +17:35:13.7
194.37951 2.41813 galactic Gem Second-epoch detections are separated by 4.6" 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 J096.3847+17.5919 | 06:25:31.30 +17:35:33.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.3847+17.5919,2461128.6223,14.04,0.05,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 J096.3847+17.5919 20260329.1223 14.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:33.68 +17:35:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.02 05:56:04.67 +16:54:40.0
191.57560 -4.07426 galactic Ori Second-epoch detections are separated by 2.5" 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 3349776802406550784 | 05:56:01.63 +16:54:41.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1931AnHar.100...61C HD 249308
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 29.1223* 05 56 04.67 +16 54 40.0 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349776802406550784,2461128.6223,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3349776802406550784 20260329.1223 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:04.67 +16:54:40.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.85 05:59:56.19 +11:30:34.1
196.75314 -5.93191 galactic Ori 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 | Gaia DR3 3342200617534182784 | 05:59:55.07 +11:30:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1931AnHar.100...61C HD 250142
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 29.1223* 05 59 56.19 +11 30 34.1 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3342200617534182784,2461128.6223,13.85,0.05,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 3342200617534182784 20260329.1223 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:56.19 +11:30:34.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 17 11.51 +12 04 06.2 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J061711.42+120425.1,2461128.6223,13.70,0.05,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
ZTF J061711.42+120425.1 20260329.1223 13.70CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:11.51 +12:04:06.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.81 06:23:49.20 +16:28:13.7
195.17342 1.52894 galactic Ori Second-epoch detections are separated by 0.3" 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 | EPIC 202083480 | 06:23:50.26 +16:27:36.4 (Gaia DR3) | VAR (local) | (local) | 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 29.1223* 06 23 49.20 +16 28 13.7 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 202083480,2461128.6223,13.81,0.05,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
EPIC 202083480 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:49.20 +16:28:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 50 25.64 +14 39 13.4 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6223,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.1223 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:25.64 +14:39:13.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.89 05:59:14.49 +14:14:26.2
194.28011 -4.73818 galactic Ori Second-epoch detections are separated by 0.9" 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 | ATO J089.8002+14.2257 | 05:59:14.42 +14:13:49.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 (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 29.1223* 05 59 14.49 +14 14 26.2 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.8002+14.2257,2461128.6223,13.89,0.05,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
ATO J089.8002+14.2257 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:14.49 +14:14:26.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.97 06:11:59.01 +17:22:43.5
193.03138 -0.53297 galactic Ori Second-epoch detections are separated by 0.7" 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 | Gaia DR3 3373213305067527296 | 06:12:00.82 +17:22:30.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE
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 29.1223* 06 11 59.01 +17 22 43.5 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3373213305067527296,2461128.6223,13.97,0.05,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 3373213305067527296 20260329.1223 13.97CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:59.01 +17:22:43.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.15 06:06:48.49 +16:49:38.2
192.91592 -1.88205 galactic Ori Second-epoch detections are separated by 0.8" and 5.5 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 3349206602545981440 | 06:06:48.48 +16:50:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 06 48.49 +16 49 38.2 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349206602545981440,2461128.6223,14.15,0.05,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
Gaia DR3 3349206602545981440 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:48.49 +16:49:38.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.04 06:24:49.25 +16:41:34.4
195.08877 1.84487 galactic Ori Second-epoch detections are separated by 2.3" 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 | Gaia DR3 3369561689514706304 | 06:24:48.37 +16:41:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.766+/- (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 24 49.25 +16 41 34.4 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3369561689514706304,2461128.6223,14.04,0.05,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 3369561689514706304 20260329.1223 14.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:24:49.25 +16:41:34.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 04 31.59 +15 26 09.2 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060431.59+152602.2,2461128.6223,13.95,0.05,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
ASASSN-V J060431.59+152602.2 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:31.59 +15:26:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.99 06:14:21.65 +14:20:39.0
195.96937 -1.48512 galactic Ori Second-epoch detections are separated by 1.4" 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 | Gaia DR3 3344797659701059328 | 06:14:19.72 +14:20:40.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1959ApJS....4...23M LF 8 +14 167
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 29.1223* 06 14 21.65 +14 20 39.0 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344797659701059328,2461128.6223,13.99,0.05,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 3344797659701059328 20260329.1223 13.99CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:21.65 +14:20:39.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.16 06:14:07.62 +18:00:35.7
192.72230 0.21767 galactic Ori Second-epoch detections are separated by 1.2" 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 | Gaia DR3 3373364999016141568 | 06:14:05.51 +18:00:23.3 (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!
TCP 2026 03 29.1223* 06 14 07.62 +18 00 35.7 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3373364999016141568,2461128.6223,14.16,0.05,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 3373364999016141568 20260329.1223 14.16CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:07.62 +18:00:35.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.06 06:01:42.11 +16:14:30.9
192.82740 -3.23574 galactic Ori Second-epoch detections are separated by 1.5" 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 | target | 06:01:42.11 +16:14:30.9 (user input) | T | P | (position from user input) SpType: A2V (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 29.1223* 06 01 42.11 +16 14 30.9 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:42.11 +16:14:30.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.03 06:20:01.74 +13:52:51.3
197.02954 -0.49536 galactic Ori Second-epoch detections are separated by 1.6" 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 J095.0104+13.8731 | 06:20:03.22 +13:52:28.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (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 29.1223* 06 20 01.74 +13 52 51.3 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.0104+13.8731,2461128.6223,14.03,0.05,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
ATO J095.0104+13.8731 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:01.74 +13:52:51.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 04 26.30 +18 02 07.7 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.04,0.05,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 20260329.1223 14.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:26.30 +18:02:07.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.00 06:25:04.23 +16:36:40.2
195.18900 1.85964 galactic Ori Second-epoch detections are separated by 2.0" 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 | ATO J096.2712+16.6032 | 06:25:06.32 +16:36:22.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 25 04.23 +16 36 40.2 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.2712+16.6032,2461128.6223,14.00,0.05,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
ATO J096.2712+16.6032 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:04.23 +16:36:40.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 01 19.48 +15 34 36.6 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060119.50+153429.8,2461128.6223,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J060119.50+153429.8 20260329.1223 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:19.48 +15:34:36.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.05 05:58:27.76 +15:59:40.1
192.65793 -4.03439 galactic Ori Second-epoch detections are separated by 0.8" 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 | Gaia DR3 3348824934574492416 | 05:58:26.25 +16:00:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1931AnHar.100...61C HD 249793
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 29.1223* 05 58 27.76 +15 59 40.1 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348824934574492416,2461128.6223,14.05,0.05,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 3348824934574492416 20260329.1223 14.05CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:27.76 +15:59:40.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.95 06:10:54.56 +14:51:53.8
195.11171 -1.96835 galactic Ori Second-epoch detections are separated by 1.1" 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 3345633533354629504 | 06:10:53.83 +14:51:21.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1959ApJS....4...23M LF 8 +14 76
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 29.1223* 06 10 54.56 +14 51 53.8 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345633533354629504,2461128.6223,13.95,0.05,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
Gaia DR3 3345633533354629504 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:54.56 +14:51:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 59 32.63 +13 11 26.7 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.03,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:32.63 +13:11:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 18 42.41 +17 53 58.5 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3370685733996143616,2461128.6223,14.04,0.05,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 3370685733996143616 20260329.1223 14.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:42.41 +17:53:58.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.91 06:19:02.13 +16:47:08.0
194.35622 0.66565 galactic Ori Second-epoch detections are separated by 1.7" 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 | ATO J094.7504+16.7831 | 06:19:00.05 +16:47:11.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B6 (LAMOST DR5) J-Ks=0.880+/-0.302 (M)
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 29.1223* 06 19 02.13 +16 47 08.0 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.7504+16.7831,2461128.6223,13.91,0.05,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
ATO J094.7504+16.7831 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:02.13 +16:47:08.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.04 05:56:16.27 +12:14:41.5
195.66583 -6.35164 galactic Ori Second-epoch detections are separated by 3.7" 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 | Gaia DR3 3343061878736545792 | 05:56:17.61 +12:14:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 56 16.27 +12 14 41.5 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3343061878736545792,2461128.6223,14.04,0.05,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 3343061878736545792 20260329.1223 14.04CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:16.27 +12:14:41.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 51 31.58 +15 47 51.0 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.18,0.05,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 20260329.1223 14.18CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:31.58 +15:47:51.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.03 06:20:39.35 +13:04:20.9
197.81437 -0.74216 galactic Ori Second-epoch detections are separated by 0.9" and 5.5 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 3332422312733018368 | 06:20:39.95 +13:04:35.5 (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 29.1223* 06 20 39.35 +13 04 20.9 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3332422312733018368,2461128.6223,14.03,0.05,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
Gaia DR3 3332422312733018368 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:39.35 +13:04:20.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 15 27.39 +14 45 49.8 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344837383856970368,2461128.6223,14.05,0.05,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 3344837383856970368 20260329.1223 14.05CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:27.39 +14:45:49.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.97 05:57:29.25 +10:49:42.8
197.05458 -6.78905 galactic Ori 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 | Gaia DR3 3342011291078406016 | 05:57:30.29 +10:49:14.9 (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 29.1223* 05 57 29.25 +10 49 42.8 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3342011291078406016,2461128.6223,13.97,0.05,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 3342011291078406016 20260329.1223 13.97CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:29.25 +10:49:42.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 10 28.12 +13 50 01.6 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061028.07+134954.2,2461128.6223,14.07,0.05,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
ASASSN-V J061028.07+134954.2 20260329.1223 14.07CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:28.12 +13:50:01.6 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.08 05:50:15.64 +13:10:20.9
194.12122 -7.16175 galactic Tau Second-epoch detections are separated by 3.0" 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 | ATO J087.5719+13.1796 | 05:50:15.40 +13:10:46.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 05 50 15.64 +13 10 20.9 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
ATO J087.5719+13.1796,2461128.6223,14.08,0.05,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 J087.5719+13.1796 20260329.1223 14.08CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:15.64 +13:10:20.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.99 06:13:50.81 +14:44:31.5
195.56025 -1.40427 galactic Ori 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 3344880917645606144 | 06:13:53.08 +14:44:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1959ApJS....4...23M LF 8 +14 153
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 29.1223* 06 13 50.81 +14 44 31.5 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344880917645606144,2461128.6223,13.99,0.05,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 3344880917645606144 20260329.1223 13.99CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:50.81 +14:44:31.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.12 06:07:09.40 +16:42:46.9
193.05640 -1.86472 galactic Ori Second-epoch detections are separated by 1.2" 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 | ATO J091.7968+16.7013 | 06:07:09.15 +16:42:12.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 06 07 09.40 +16 42 46.9 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.7968+16.7013,2461128.6223,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.7968+16.7013 20260329.1223 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:09.40 +16:42:46.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.03 06:25:46.57 +17:09:24.5
194.78459 2.26323 galactic Gem Second-epoch detections are separated by 1.0" 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 J096.4429+17.1515 | 06:25:46.57 +17:09:24.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J096.4429+17.1515,2461128.6223,14.03,0.05,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
ATO J096.4429+17.1515 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:46.57 +17:09:24.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.07 05:59:11.19 +16:41:15.8
192.14075 -3.53998 galactic Ori Second-epoch detections are separated by 2.5" 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 3348978621387560832 | 05:59:08.44 +16:41:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 59 11.19 +16 41 15.8 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348978621387560832,2461128.6223,14.07,0.05,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 3348978621387560832 20260329.1223 14.07CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:11.19 +16:41:15.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 13.97 06:26:02.09 +15:47:59.3
196.01514 1.68630 galactic Gem Second-epoch detections are separated by 2.9" 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 | ATO J096.4996+15.7999 | 06:25:59.91 +15:47:59.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.4996+15.7999,2461128.6223,13.97,0.05,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
ATO J096.4996+15.7999 20260329.1223 13.97CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:02.09 +15:47:59.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 58 52.27 +13 37 22.3 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.14,0.05,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
target 20260329.1223 14.14CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:52.27 +13:37:22.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.19 05:51:44.60 +15:34:43.5
192.20906 -5.64241 galactic Tau Second-epoch detections are separated by 1.0" 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 | target | 05:51:44.60 +15:34:43.5 (user input) | T | P | (position from user input) J-Ks=1.058+/- (M)
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 29.1223* 05 51 44.60 +15 34 43.5 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.19,0.05,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
target 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:44.60 +15:34:43.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.05 05:51:19.82 +13:57:03.9
193.57401 -6.54641 galactic Tau Second-epoch detections are separated by 2.6" and 5.6 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 | ASASSN-V J055121.04+135629.9 | 05:51:21.04 +13:56:29.9 (Gaia DR3) | SR (local) | 156.000000000000 (local) | Gaia3var=VARIABLE
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 29.1223* 05 51 19.82 +13 57 03.9 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
ASASSN-V J055121.04+135629.9,2461128.6223,14.05,0.05,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
ASASSN-V J055121.04+135629.9 20260329.1223 14.05CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:19.82 +13:57:03.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 13 47.44 +15 24 03.1 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.08,0.05,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 20260329.1223 14.08CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:47.44 +15:24:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.21 06:16:28.87 +15:12:39.8
195.45136 -0.62143 galactic Ori Second-epoch detections are separated by 3.0" 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 | Gaia DR3 3345018150440472448 | 06:16:30.10 +15:12:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1959ApJS....4...23M LF 8 +15 153
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 29.1223* 06 16 28.87 +15 12 39.8 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3345018150440472448,2461128.6223,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3345018150440472448 20260329.1223 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:28.87 +15:12:39.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.31 06:01:20.72 +17:26:15.5
191.74345 -2.72071 galactic Ori Second-epoch detections are separated by 0.5" 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 | Gaia DR3 3350156954252096896 | 06:01:23.59 +17:26:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1931AnHar.100...61C HD 250394
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 29.1223* 06 01 20.72 +17 26 15.5 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3350156954252096896,2461128.6223,14.31,0.05,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 3350156954252096896 20260329.1223 14.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:20.72 +17:26:15.5 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.18 05:55:50.23 +17:41:16.2
190.87257 -3.73568 galactic Ori 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 | 05:55:50.23 +17:41:16.2 (user input) | T | P | (position from user input) SpType: K1 (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 29.1223* 05 55 50.23 +17 41 16.2 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.18,0.05,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 20260329.1223 14.18CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:50.23 +17:41:16.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:42.81 +17:46:45.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.27 06:19:59.21 +17:10:05.3
194.12638 1.04683 galactic Ori Second-epoch detections are separated by 0.6" 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 | ATO J094.9970+17.1664 | 06:19:57.50 +17:10:24.5 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | 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 29.1223* 06 19 59.21 +17 10 05.3 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.9970+17.1664,2461128.6223,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.9970+17.1664 20260329.1223 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:59.21 +17:10:05.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.25 05:52:03.63 +15:17:57.9
192.49032 -5.71681 galactic Tau Second-epoch detections are separated by 0.6" 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 | Gaia DR3 3348008130574331904 | 05:52:03.64 +15:17:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 52 03.63 +15 17 57.9 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348008130574331904,2461128.6223,14.25,0.05,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 3348008130574331904 20260329.1223 14.25CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:03.63 +15:17:57.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 52 24.06 +13 07 42.1 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:24.06 +13:07:42.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.41 05:57:35.03 +15:59:00.1
192.56251 -4.22327 galactic Ori 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 | ATO J089.3971+15.9860 | 05:57:35.03 +15:59:00.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 57 35.03 +15 59 00.1 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.3971+15.9860,2461128.6223,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.3971+15.9860 20260329.1223 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:35.03 +15:59:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 57 42.27 +15 57 13.2 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348823658966427392,2461128.6223,14.38,0.05,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
Gaia DR3 3348823658966427392 20260329.1223 14.38CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:42.27 +15:57:13.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 02 07.56 +15 11 23.2 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:07.56 +15:11:23.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.29 06:13:10.18 +12:55:19.3
197.08114 -2.41874 galactic Ori Second-epoch detections are separated by 2.4" 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 | Gaia DR3 3344086000799337344 | 06:13:11.97 +12:55:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 13 10.18 +12 55 19.3 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344086000799337344,2461128.6223,14.29,0.05,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
Gaia DR3 3344086000799337344 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:10.18 +12:55:19.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.27 05:59:54.48 +16:54:38.7
192.03229 -3.27952 galactic Ori Second-epoch detections are separated by 1.8" 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 | Gaia DR3 3348989066746631552 | 05:59:51.84 +16:54:44.1 (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 29.1223* 05 59 54.48 +16 54 38.7 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348989066746631552,2461128.6223,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3348989066746631552 20260329.1223 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:54.48 +16:54:38.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.31 06:19:36.57 +17:40:29.3
193.63709 1.20653 galactic Ori Second-epoch detections are separated by 0.7" 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 3370664499677963520 | 06:19:39.47 +17:40:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (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 29.1223* 06 19 36.57 +17 40 29.3 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3370664499677963520,2461128.6223,14.31,0.05,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 3370664499677963520 20260329.1223 14.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:36.57 +17:40:29.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.29 06:20:16.95 +13:20:08.4
197.53940 -0.69824 galactic Ori Second-epoch detections are separated by 3.0" 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 | 06:20:16.95 +13:20:08.4 (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 29.1223* 06 20 16.95 +13 20 08.4 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.29,0.05,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 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:16.95 +13:20:08.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.41 05:55:56.82 +17:18:04.4
191.22121 -3.90639 galactic Ori Second-epoch detections are separated by 1.6" 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 | ATO J088.9820+17.3144 | 05:55:56.21 +17:18:38.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K4 (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 29.1223* 05 55 56.82 +17 18 04.4 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.9820+17.3144,2461128.6223,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.9820+17.3144 20260329.1223 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:56.82 +17:18:04.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 55 03.80 +15 54 25.8 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3349561332487777664,2461128.6223,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3349561332487777664 20260329.1223 14.48CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:03.80 +15:54:25.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 58 30.34 +17 44 47.9 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.47,0.05,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
target 20260329.1223 14.47CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:30.34 +17:44:47.9 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.32 05:57:06.30 +17:40:03.3
191.04133 -3.48420 galactic Ori Second-epoch detections are separated by 1.5" 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 | 05:57:06.30 +17:40:03.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 57 06.30 +17 40 03.3 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:06.30 +17:40:03.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.19 06:27:31.25 +15:16:12.9
196.65070 1.75683 galactic Gem Second-epoch detections are separated by 0.7" 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 | ATO J096.8852+15.2532 | 06:27:31.89 +15:15:39.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.8852+15.2532,2461128.6223,14.19,0.05,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
ATO J096.8852+15.2532 20260329.1223 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:31.25 +15:16:12.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.30 05:50:07.25 +15:27:57.1
192.10901 -6.03686 galactic Tau Second-epoch detections are separated by 1.2" and 5.6 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 3348074895845499392 | 05:50:07.79 +15:27:18.3 (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!
TCP 2026 03 29.1223* 05 50 07.25 +15 27 57.1 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348074895845499392,2461128.6223,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3348074895845499392 20260329.1223 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:07.25 +15:27:57.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.38 05:56:47.22 +17:56:00.9
190.77257 -3.41702 galactic Ori Second-epoch detections are separated by 1.7" 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 | ATO J089.2033+17.9415 | 05:56:47.97 +17:56:30.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1223* 05 56 47.22 +17 56 00.9 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2033+17.9415,2461128.6223,14.38,0.05,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
ATO J089.2033+17.9415 20260329.1223 14.38CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:47.22 +17:56:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.52 06:04:09.22 +15:25:54.2
193.82420 -3.11922 galactic Ori Second-epoch detections are separated by 2.3" 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 | ATO J091.0295+15.4235 | 06:04:09.22 +15:25:54.2 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1223* 06 04 09.22 +15 25 54.2 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.0295+15.4235,2461128.6223,14.52,0.05,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 J091.0295+15.4235 20260329.1223 14.52CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:09.22 +15:25:54.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 57 37.01 +16 32 37.8 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.43,0.05,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 20260329.1223 14.43CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:37.01 +16:32:37.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.23 06:18:00.48 +17:37:01.4
193.50754 0.84304 galactic Ori Second-epoch detections are separated by 1.0" 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 | 06:18:00.48 +17:37:01.4 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 18 00.48 +17 37 01.4 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.23,0.05,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 20260329.1223 14.23CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:00.48 +17:37:01.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 48 37.32 +15 50 58.7 14.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348290567623766144,2461128.6223,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3348290567623766144 20260329.1223 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:37.32 +15:50:58.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.49 05:51:06.30 +15:03:04.4
192.58943 -6.04090 galactic Tau Second-epoch detections are separated by 1.7" 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 J087.7706+15.0575 | 05:51:06.30 +15:03:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 51 06.30 +15 03 04.4 14.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.7706+15.0575,2461128.6223,14.49,0.05,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 J087.7706+15.0575 20260329.1223 14.49CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:06.30 +15:03:04.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.38 05:56:09.13 +17:46:33.2
190.83377 -3.62668 galactic Ori Second-epoch detections are separated by 2.0" 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 | ATO J089.0407+17.7839 | 05:56:09.13 +17:46:33.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 56 09.13 +17 46 33.2 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.0407+17.7839,2461128.6223,14.38,0.05,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
ATO J089.0407+17.7839 20260329.1223 14.38CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:09.13 +17:46:33.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.21 06:05:46.85 +10:58:59.2
197.91479 -4.93526 galactic Ori Second-epoch detections are separated by 0.9" 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 J091.4447+10.9811 | 06:05:46.85 +10:58:59.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 05 46.85 +10 58 59.2 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.4447+10.9811,2461128.6223,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.4447+10.9811 20260329.1223 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:46.85 +10:58:59.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.44 06:02:07.79 +16:23:46.6
192.74340 -3.07039 galactic Ori Second-epoch detections are separated by 2.3" and 5.6 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 | ASAS J060205+1623.7 | 06:02:05.19 +16:23:45.5 (Gaia DR3) | ESD/DCEP- (local) | 2452623.44000 (local) | Gaia3var=VARIABLE SpType: A1V (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 29.1223* 06 02 07.79 +16 23 46.6 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J060205+1623.7,2461128.6223,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J060205+1623.7 20260329.1223 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:07.79 +16:23:46.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.53 06:06:25.19 +16:38:04.6
193.03904 -2.05705 galactic Ori Second-epoch detections are separated by 0.8" 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 | 06:06:25.19 +16:38:04.6 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 06 25.19 +16 38 04.6 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:25.19 +16:38:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.31 05:55:23.29 +14:46:09.8
193.35515 -5.28624 galactic Ori Second-epoch detections are separated by 2.2" 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 | ATO J088.8515+14.7824 | 05:55:23.04 +14:46:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K4 (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 29.1223* 05 55 23.29 +14 46 09.8 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.8515+14.7824,2461128.6223,14.31,0.05,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 J088.8515+14.7824 20260329.1223 14.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:23.29 +14:46:09.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 54 30.03 +14 48 43.8 14.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.61,0.05,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
target 20260329.1223 14.61CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:30.03 +14:48:43.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 51 14.90 +14 02 32.7 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.35,0.05,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
target 20260329.1223 14.35CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:14.90 +14:02:32.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 20 35.52 +13 38 05.2 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:35.52 +13:38:05.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.42 05:56:33.13 +15:24:54.7
192.93322 -4.72114 galactic Ori Second-epoch detections are separated by 1.1" 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 | Gaia DR3 3348732021545094272 | 05:56:31.18 +15:25:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1931AnHar.100...61C HD 249428
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 29.1223* 05 56 33.13 +15 24 54.7 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3348732021545094272,2461128.6223,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3348732021545094272 20260329.1223 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:33.13 +15:24:54.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.42 06:18:21.39 +17:01:39.7
194.06603 0.63713 galactic Ori Second-epoch detections are separated by 1.7" 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 | ATO J094.5958+17.0217 | 06:18:21.39 +17:01:39.7 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1223* 06 18 21.39 +17 01 39.7 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.5958+17.0217,2461128.6223,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.5958+17.0217 20260329.1223 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:21.39 +17:01:39.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.37 05:59:25.67 +15:07:24.7
193.53210 -4.26331 galactic Ori Second-epoch detections are separated by 0.3" 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 | 05:59:25.67 +15:07:24.7 (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 29.1223* 05 59 25.67 +15 07 24.7 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:25.67 +15:07:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.49 05:56:40.30 +16:06:18.8
192.34719 -4.35279 galactic Ori Second-epoch detections are separated by 1.8" and 5.7 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 | 05:56:40.30 +16:06:18.8 (user input) | T | P | (position from user input) SpType: G0 (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 29.1223* 05 56 40.30 +16 06 18.8 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.49,0.05,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 20260329.1223 14.49CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:40.30 +16:06:18.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.45 06:01:21.00 +12:23:32.8
196.14907 -5.19864 galactic Ori Second-epoch detections are separated by 1.6" 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 | ATO J090.3379+12.4030 | 06:01:21.00 +12:23:32.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 01 21.00 +12 23 32.8 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.3379+12.4030,2461128.6223,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.3379+12.4030 20260329.1223 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:21.00 +12:23:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 09 30.91 +13 08 59.7 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.38,0.05,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 20260329.1223 14.38CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:30.91 +13:08:59.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 59 57.80 +17 18 57.4 14.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.60,0.05,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 20260329.1223 14.60CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:57.80 +17:18:57.4 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.60 05:50:27.70 +15:04:18.3
192.49293 -6.16473 galactic Tau Second-epoch detections are separated by 0.2" and 5.5 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 | ATO J087.6153+15.0696 | 05:50:27.70 +15:04:18.3 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1223* 05 50 27.70 +15 04 18.3 14.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.6153+15.0696,2461128.6223,14.60,0.05,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 J087.6153+15.0696 20260329.1223 14.60CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:27.70 +15:04:18.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.46 05:53:11.70 +14:46:13.7
193.08830 -5.74508 galactic Ori Second-epoch detections are separated by 1.4" 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 | ATO J088.3061+14.7656 | 05:53:11.70 +14:46:13.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 05 53 11.70 +14 46 13.7 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.3061+14.7656,2461128.6223,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.3061+14.7656 20260329.1223 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:11.70 +14:46:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 18 51.02 +14 40 00.2 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3344749903963079808,2461128.6223,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3344749903963079808 20260329.1223 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:51.02 +14:40:00.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.51 05:56:00.89 +15:07:20.7
193.12340 -4.97922 galactic Ori Second-epoch detections are separated by 1.0" 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 | 05:56:00.89 +15:07:20.7 (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 29.1223* 05 56 00.89 +15 07 20.7 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.51,0.05,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
target 20260329.1223 14.51CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:00.89 +15:07:20.7 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.31 06:21:30.97 +15:43:18.3
195.57516 0.68901 galactic Ori Second-epoch detections are separated by 0.4" 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 | ATO J095.3815+15.7117 | 06:21:30.97 +15:43:18.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 21 30.97 +15 43 18.3 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.3815+15.7117,2461128.6223,14.31,0.05,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 J095.3815+15.7117 20260329.1223 14.31CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:30.97 +15:43:18.3 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.61 06:10:55.00 +17:26:53.0
192.84813 -0.72268 galactic Ori Second-epoch detections are separated by 1.0" 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 3373228625213998336 | 06:10:52.77 +17:26:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1223* 06 10 55.00 +17 26 53.0 14.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3373228625213998336,2461128.6223,14.61,0.05,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 3373228625213998336 20260329.1223 14.61CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:55.00 +17:26:53.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 06 15 16.16 +15 59 57.2 14.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1223 14.52CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:16.16 +15:59:57.2 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 49 48.99 +11 48 49.0 14.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6223,14.57,0.05,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 20260329.1223 14.57CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:48.99 +11:48:49.0 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1223 2461128.6223 14.30 06:21:23.34 +13:14:45.8
197.74527 -0.50297 galactic Ori Second-epoch detections are separated by 1.0" 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 | Gaia DR3 3332431869040001152 | 06:21:22.61 +13:14:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1959ApJS....4...23M LF 8 +13 317
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 29.1223* 06 21 23.34 +13 14 45.8 14.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3332431869040001152,2461128.6223,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332431869040001152 20260329.1223 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:23.34 +13:14:45.8 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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 29.1223* 05 58 23.72 +11 50 43.1 13.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6223,13.70,0.05,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 20260329.1223 13.70CV 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:23.72 +11:50:43.1 ;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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20_00sec_-15_00C_LIGHT_0057_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: 2461093.62619102 22.02.2026 03:01:32.904 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
First image: 2461093.62619102 22.02.2026 03:01:32.904 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
Last image: 2461128.62257323 29.03.2026 02:56:20.327 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
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: 12 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): 27068
Objects passed selection criteria: 26971
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 21048.8
Average stars matched: 20510.2 (97.4417 %)
Memory usage VmPeak: 131560 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 28 22:00:07 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: 2461093.62619102 22.02.2026 03:01:32.904 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
First image: 2461093.62619102 22.02.2026 03:01:32.904 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
Last image: 2461128.62257323 29.03.2026 02:56:20.327 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1404
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 179 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): 156499
Objects passed selection criteria: 156213
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 138648
Average stars matched: 133130 (96.0207 %)
Memory usage VmPeak: 1979508 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 28 22:04:34 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
SExtractor catalog cache: saved Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.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: 2461128.62198786
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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits'
wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
Saving wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits'
wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits exists and is non-empty
Saving wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits'
wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
Saving wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:12:57.578 +14:00:50.20
Second-epoch image center 06:13:26.716 +14:00:59.74
Angular distance between the image centers 0.12 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 06:12:57.578 +14:00:50.20
Second-epoch image center 06:13:25.832 +14:01:27.76
Angular distance between the image centers 0.11 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 06:13:26.716 +14:00:59.74
Second-epoch second image center 06:13:25.832 +14:01:27.76
Angular distance between the image centers 0.00856 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits &> /tmp/tmp.rRKfcOlzar
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.AUAyMomBcp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits &> /tmp/tmp.ou58dnf38X
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.dbQE9M2wT8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits and wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits and wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
Found non-empty wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits and wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
The reference image (wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits) and catalog (wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat) found
'wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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 14445 out of 32217 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.982813
a=0.000000 b=1.000000 c=22.982813
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.9 pix Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
2.9 pix Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
2.4 pix fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
2.3 pix fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Limiting magnitude estimates:
15.0 mag. Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
15.0 mag. Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
14.4 mag. fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
14.4 mag. fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rRKfcOlzar (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
Checking if the catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS catalog name: wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3172, passed=32217
Got 32217 stars (including 29017 good ones) from the SExtractor catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 32217 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 917 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: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.82"
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 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.83"
Estimated accuracy of the plate solution: 0.93"
Excluding outliers - 911 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits -region wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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.AUAyMomBcp (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3211, passed=32051
Got 32051 stars (including 28826 good ones) from the SExtractor catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 32051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 921 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: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.83"
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 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.84"
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.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.ou58dnf38X (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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1512, passed=16378
Got 16378 stars (including 14841 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat
util/solve_plate_with_UCAC5 got 16378 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 914 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits -region wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.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.dbQE9M2wT8 (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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1552, passed=16305
Got 16305 stars (including 14734 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 16305 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 920 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits'
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits'
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits'
Preparing the HTML report for the field Ori-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out51986.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 51571_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51571_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:39:44.92 +13:43:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.17, MAG_FAINT_SEARCH_LIMIT=12.15)GAIADR2_OUTPUT=# 2.667 3355774947574055680 099.93724959274 +13.73068018458 11.0500 10.3778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51572_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51572_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:53.73 +14:54:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 2.940 3356239285078194176 099.47425692088 +14.91568822201 10.8651 10.0886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51574_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51574_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:41.68 +16:32:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 2.888 3369541211110732672 096.42382454315 +16.54082334187 10.9869 10.2679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51576_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51576_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:25.68 +16:03:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 3.328 3357845053090488832 100.35714121559 +16.06408544540 11.0387 10.6139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51578_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51578_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:26.90 +17:16:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 2.346 3349986323792979328 088.86212951416 +17.27215543188 11.0935 10.8277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51581_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51581_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:18.73 +14:00:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.07, MAG_FAINT_SEARCH_LIMIT=10.05)GAIADR2_OUTPUT=# 1.943 3345194347178716800 092.07770715289 +14.00376444567 8.3071 7.1898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51582_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51582_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:32.05 +13:58:00.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 51670_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51670_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:18.77 +13:59:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.14, MAG_FAINT_SEARCH_LIMIT=11.12)GAIADR2_OUTPUT=# 3.046 3345194347176271872 092.07802470555 +13.98856167066 10.5449 10.4762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51679_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51679_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:15.40 +15:33:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 1.934 3345750115942949120 092.81452392098 +15.56272641147 10.3958 9.9883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51722_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51722_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:25.27 +15:43:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 1.075 3357096216952323968 098.85533171442 +15.71842612673 10.4561 9.7252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51759_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51759_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:05.09 +15:12:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 3.333 3348478657131124480 090.52162924754 +15.19941809654 10.6687 9.8662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51843_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51843_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:59.94 +18:04:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 3.143 3350286009430416896 090.75017501953 +18.06644822458 11.2410 11.0507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51858_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51858_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:11.73 +16:02:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 3.687 3369842614734207616 094.04896400037 +16.03272934948 11.3241 10.9135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51880_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51880_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:52.06 +14:13:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51947_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 51947_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:43.82 +16:47:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 2.777 3369392296004628736 096.93299990475 +16.78342297646 10.8171 9.7201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51986_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 51986_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 52006_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 52006_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:19.03 +17:40:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 3.357 3350026528984261632 089.07931686384 +17.66681788967 11.5881 10.9490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.357#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: 7s
Prepared the HTML report for the field Ori-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:35:44.72 +11:17:02.2
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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
SExtractor catalog cache: saved Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits exists and is non-empty
wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits exists and is non-empty
wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:12:57.578 +14:00:50.20
Second-epoch image center 06:13:26.716 +14:00:59.74
Angular distance between the image centers 0.12 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 06:12:57.578 +14:00:50.20
Second-epoch image center 06:13:25.832 +14:01:27.76
Angular distance between the image centers 0.11 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 06:13:26.716 +14:00:59.74
Second-epoch second image center 06:13:25.832 +14:01:27.76
Angular distance between the image centers 0.00856 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/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits &> /tmp/tmp.rJPUhnuY8v
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.d1dg1If5cO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits &> /tmp/tmp.9tenHu1nMb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.Y5qEwXiMvv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits and wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits and wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
Found non-empty wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits and wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
The reference image (wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits) and catalog (wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat) found
'wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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 14977 out of 175673 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.809799
a=0.000000 b=1.000000 c=22.809799
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.18
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1062 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.6 pix Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
2.5 pix Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
2.1 pix fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
2.1 pix fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Limiting magnitude estimates:
15.2 mag. Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
15.2 mag. Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
14.6 mag. fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
14.6 mag. fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rJPUhnuY8v (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
Checking if the catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS catalog name: wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=30781, passed=175640
Got 175640 stars (including 144699 good ones) from the SExtractor catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 175640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 916 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: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
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 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.77"
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits -region wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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.d1dg1If5cO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=31217, passed=177894
Got 177894 stars (including 146501 good ones) from the SExtractor catalog wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 177894 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 917 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: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
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 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.77"
Estimated accuracy of the plate solution: 0.87"
Excluding outliers - 908 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.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.9tenHu1nMb (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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=12423, passed=129331
Got 129331 stars (including 116731 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat
util/solve_plate_with_UCAC5 got 129331 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 906 stars left (next iteration limit 995)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits -region wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.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.Y5qEwXiMvv (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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=12548, passed=130255
Got 130255 stars (including 117542 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 130255 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 913 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 908 stars left (next iteration limit 996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits
Saving fully-calibrated image wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/wcs_Ori-02-Q2b1x1_2026-02-21_21-02-20_20.00sec_-15.00C_LIGHT_0045.fits
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.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_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-55-29_20.00sec_-15.00C_LIGHT_0057.fits
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_215734_TTUQ2b1x1_21212_HgZ0VJyV/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058.fits
Preparing the HTML report for the field Ori-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out200033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200839.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out200067.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200297.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200306.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200363.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200395.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200444.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200447.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200488.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200499.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200523.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200527.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200540.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200547.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200563.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200580.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200614.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200622.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200668.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200672.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200676.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200745.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200778.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200792.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200881.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out201358.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out201832.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out201962.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202499.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202516.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202524.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202809.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202913.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202988.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202990.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203074.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203133.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203155.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203170.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203283.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203340.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203413.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203420.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203492.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203582.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203598.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203745.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203757.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203768.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203779.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203847.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204012.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204057.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204072.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204095.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204160.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204170.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204267.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204567.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204665.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204691.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204886.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204946.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204981.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205151.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205296.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205336.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205361.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205589.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out124797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202952.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203383.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203645.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203672.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203926.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203969.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204000.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204029.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204123.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204177.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204520.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204540.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204603.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205021.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205231.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205256.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205430.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205439.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205574.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 487s
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: 202s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200033_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200033_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:24.91 +10:20:18.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200039_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200039_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200048_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200048_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:08.61 +11:12:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 5.666 3342306170650986240 091.03568572040 +11.21390929187 14.5025 13.8789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200054_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200054_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200057_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200057_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200061_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200061_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200065_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200065_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200067_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200067_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:28.54 +15:07:56.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 200070_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200070_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200075_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200075_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:03.85 +13:39:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 5.297 3343763264076253568 089.51678625891 +13.66127424215 14.2613 13.7429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200078_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200078_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200083_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200083_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:07.10 +17:11:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 5.618 3370028226041229440 095.27942090629 +17.19003051495 14.3824 13.5499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200093_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200093_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200096_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200096_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200103_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200103_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200116_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200116_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:57.21 +13:39:20.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)
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Considering the candidate 200120_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200120_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:01.33 +13:57:12.0 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 200123_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200123_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200124_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200124_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200130_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200130_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:33.75 +13:33:16.1 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 200135_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200135_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200144_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200144_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200148_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200148_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 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 200149_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200149_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200150_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200150_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200151_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200151_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200162_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200162_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 200172_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200172_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:20:01.88 +17:49:58.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)
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Considering the candidate 200173_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200173_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200177_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200177_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200181_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200181_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200189_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200189_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:41.69 +12:31:16.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)
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Considering the candidate 200191_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200191_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200192_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200192_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200194_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200194_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200198_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200198_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200199_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200199_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200207_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200207_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 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 200208_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200208_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:05.18 +10:12:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 4.892 3335950787282602880 089.02060516119 +10.21331874673 13.9806 13.4126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200209_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200209_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200211_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200211_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200212_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200212_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200213_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200213_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200216_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200216_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:51.55 +11:36:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 4.644 3330374957661609216 092.46453520989 +11.61054037953 14.1349 13.3010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200219_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200219_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200220_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200220_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:09.04 +15:05:39.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
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Considering the candidate 200224_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200224_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200241_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200241_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200242_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200242_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:40.90 +15:54:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 5.275 3348116436768831744 087.92057419324 +15.90129269416 14.1517 13.3672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200256_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200256_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200260_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200260_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200261_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200261_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200263_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200263_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:22.12 +14:41:38.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
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Considering the candidate 200265_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200265_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:42.58 +14:00:25.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)
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Considering the candidate 200266_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200266_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:16.23 +13:31:34.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
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Considering the candidate 200267_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200267_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200276_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200276_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200279_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200279_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200280_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200280_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200285_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200285_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:28.82 +13:47:20.3 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 200288_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200288_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200292_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200292_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200295_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200295_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200297_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200297_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:26.20 +14:04:31.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)
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Considering the candidate 200298_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200298_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:32.04 +13:58:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 5.629 3345114941822822272 091.63374613282 +13.97867709645 13.7071 12.5840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200299_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200299_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:15.95 +09:44:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 5.145 3329148005765077760 094.31650454472 +09.73679389035 13.9512 13.4021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200300_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200300_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:39:47.52 +12:43:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 4.344 3352287056174108416 099.94765645620 +12.71600737825 13.9948 13.4194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200302_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200302_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:24.77 +17:22:25.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
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Considering the candidate 200306_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200306_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:17.05 +17:15:29.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)
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Considering the candidate 200311_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200311_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:07.46 +17:20:55.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)
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Considering the candidate 200316_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200316_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200317_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200317_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:47.41 +18:07:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 5.562 3371161994327905920 098.69766716342 +18.11934841627 14.0663 13.4931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200318_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200318_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200319_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200319_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:50.12 +14:00:22.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 200321_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200321_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:50.35 +14:07:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.911 3332593084932722304 095.96027472509 +14.12592429555 14.2861 13.7911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200322_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200322_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:20.11 +11:20:49.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)
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Considering the candidate 200325_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200325_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
Rejecting candidate due to large distance (30.8") between the two second-epoch detections
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Considering the candidate 200327_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200327_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200328_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200328_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200330_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200330_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:47.94 +14:30:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 4.239 3346961331084857216 089.20061927044 +14.50759305511 13.9202 13.3969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200332_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200332_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200333_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200333_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:47.47 +13:38:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200334_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200334_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200337_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200337_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200340_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200340_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200342_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200342_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200343_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200343_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:31:14.35 +13:44:26.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)
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Considering the candidate 200349_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200349_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200350_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200350_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200351_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200351_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200352_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200352_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:36.53 +13:06:44.6 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 200354_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200354_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:36.98 +12:43:06.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)
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Considering the candidate 200356_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200356_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200358_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200358_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:33.19 +11:43:33.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 200361_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200361_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:12.78 +17:42:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 5.664 3359080938519910016 099.55362038979 +17.70085558458 13.7056 12.9825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200363_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200363_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:51.14 +16:29:03.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 200368_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200368_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200370_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200370_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:38.84 +13:08:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 5.544 3343671661014384128 089.41172144014 +13.13696392680 13.8382 13.3165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200371_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200371_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:49.95 +12:52:22.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
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Considering the candidate 200372_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200372_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200373_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200373_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:12.28 +14:15:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200376_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200376_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200379_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200379_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:54.16 +15:34:32.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)
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Considering the candidate 200380_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200380_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:05:33.36 +12:13:56.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 200382_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200382_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:18:32.26 +10:16:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.960 3329207649972301440 094.63519888818 +10.27969049065 13.8487 13.4666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200385_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200385_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:16.46 +10:19:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 5.455 3336667767646600704 087.56793302196 +10.31804318937 13.9944 13.4968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200386_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200386_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200388_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200388_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:53.04 +11:45:53.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)
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Considering the candidate 200390_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200390_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200392_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200392_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:01.33 +14:55:18.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)
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Considering the candidate 200393_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200393_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:31:24.71 +16:39:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 5.748 3369410437946399488 097.85290745181 +16.66184853411 13.5992 13.0458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200395_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200395_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:24:00.39 +16:38:30.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)
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Considering the candidate 200402_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200402_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200404_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200404_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200408_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200408_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200409_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200409_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:26.85 +11:32:06.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 200411_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200411_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200412_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200412_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200415_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200415_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200416_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200416_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:39:40.26 +17:56:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 5.229 3359102413356249216 099.91708222695 +17.94583274963 14.2202 13.7467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200418_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200418_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200420_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200420_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:55.41 +14:35:28.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
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Considering the candidate 200421_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200421_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:31.27 +15:51:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 5.624 3348071322432868480 088.12995862512 +15.85205443590 13.7189 13.1804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200423_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200423_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200425_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200425_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:28.59 +16:54:48.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
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Considering the candidate 200426_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200426_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200427_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200427_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:22.42 +14:22:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 5.262 3347071969442763008 088.09315529306 +14.36778278184 13.8632 13.3093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200428_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200428_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:22.67 +17:32:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 5.210 3370435212845424128 095.84457679996 +17.53430722851 13.4854 12.5227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200431_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200431_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:48:46.34 +15:33:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 5.482 3347997483354073728 087.19279906293 +15.55408530613 13.6862 13.0663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200432_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200432_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:05:01.87 +13:09:16.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 200434_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200434_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:16.12 +10:15:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200436_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200436_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200437_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200437_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:58.78 +14:38:49.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)
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Considering the candidate 200438_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200438_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:09.47 +14:11:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 5.869 3356601672941725312 096.53922134735 +14.18433042432 13.4241 12.5177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200439_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200439_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200443_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200443_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:39.09 +17:03:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.813 3369492282842716544 097.16279143249 +17.05277609235 13.8832 13.1862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200444_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200444_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:23.22 +14:41:16.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)
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Considering the candidate 200446_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200446_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:15.56 +17:23:48.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)
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Considering the candidate 200447_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200447_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:42.15 +13:43:33.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 200449_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200449_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:06.20 +16:32:29.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 200450_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200450_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200453_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200453_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200454_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200454_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200456_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200456_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:26.28 +10:28:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.880 3341971953475312640 089.10895154592 +10.47172847434 13.8151 13.0489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200459_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200459_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200460_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200460_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:54.84 +17:54:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 5.108 3359108525093272320 099.72847075201 +17.91160924778 13.7341 13.2577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200461_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200461_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:18:47.38 +14:09:25.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 200462_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200462_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200464_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200464_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200466_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200466_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:31:37.75 +18:01:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.242 3371243255109944320 097.90689723724 +18.01862571162 14.0826 13.7250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200470_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200470_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:07.91 +14:15:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.054 3346860107295167488 088.78399670139 +14.26305030234 13.7315 13.3243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200471_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200471_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200473_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200473_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:21.90 +16:07:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200477_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200477_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:44.66 +15:28:05.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 200478_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200478_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:39:44.89 +13:48:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.237 3355801950028702976 099.93655730155 +13.81106776760 13.4117 12.5942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200480_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200480_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200481_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200481_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200483_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200483_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:57.36 +10:41:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.566 3329283962950306432 094.23856544948 +10.68383359889 13.7664 13.0423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200484_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200484_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:48:19.94 +15:50:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 5.841 3348290468844085120 087.08245569672 +15.84529946299 13.9475 13.3664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200485_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200485_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200487_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200487_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200488_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200488_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:28.00 +13:42:36.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 200489_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200489_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200491_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200491_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:05:48.76 +16:31:02.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 200493_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200493_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200495_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200495_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:03.14 +17:39:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 5.240 3350036699466846592 089.01264130404 +17.65052338538 13.5511 12.6845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200498_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200498_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:38.17 +13:18:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 5.802 3346421638376062208 087.90908230800 +13.30927773900 13.8250 13.2547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200499_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200499_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:23.67 +12:06:04.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 200500_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200500_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:33.66 +16:57:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200502_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200502_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:43.97 +15:33:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200503_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200503_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200504_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200504_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200506_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200506_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:48.94 +15:14:48.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 200507_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200507_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200510_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200510_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200512_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200512_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200514_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200514_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:05.58 +14:24:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.909 3355963097201792000 100.27322513003 +14.39913649209 13.5856 12.6941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200517_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200517_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:43.50 +10:43:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.698 3330173472156114176 092.43144433513 +10.71856770900 14.0007 13.4286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200518_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200518_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:17.65 +15:11:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 5.555 3348513738423788288 089.82372061398 +15.18188325063 13.3947 12.7590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200520_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200520_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:16.50 +12:48:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.552 3332062222674775296 093.81876494017 +12.80520788578 14.0467 13.5271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200522_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200522_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:25.85 +11:32:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.733 3342940893798771968 089.35761772927 +11.54590990372 13.4058 12.6127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200523_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200523_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:39.57 +17:48:41.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 200525_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200525_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:22.80 +13:03:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.976 3346352781462233856 088.34498553294 +13.04872890317 13.3928 12.8155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200527_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200527_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:32.75 +14:54:47.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
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Considering the candidate 200529_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200529_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200530_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200530_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:33:08.45 +16:30:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 3.936 3357404217647409536 098.28528121886 +16.50074210242 13.3486 12.4444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200532_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200532_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:27.40 +16:42:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 5.790 3349729282888241792 089.61421754491 +16.70517019713 13.5103 12.6438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200533_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200533_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:07.97 +13:41:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.724 3346452841315535104 087.78306724763 +13.69333373539 13.6435 13.1746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200536_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200536_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200538_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200538_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200540_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200540_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:27.22 +17:21:41.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 200544_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200544_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200547_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200547_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:37.88 +11:22:43.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 200549_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200549_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:06.41 +17:10:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 5.647 3358801250249246720 100.27636922721 +17.17757626340 13.7919 13.0689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200551_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200551_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200552_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200552_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:33:34.19 +17:53:05.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 200553_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200553_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:02.40 +15:30:13.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200554_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200554_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:38.18 +17:17:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200555_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200555_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200556_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200556_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:54.62 +16:03:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200557_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200557_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200559_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200559_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:19.40 +13:58:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.208 3343889845352593536 090.08057899541 +13.96744067355 13.6876 13.1653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200562_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200562_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200563_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200563_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:59.26 +12:18:18.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200566_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200566_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200567_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200567_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:17.46 +09:59:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.621 3341707658367979520 090.32255788627 +09.98884150676 13.5265 13.0828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200569_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200569_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:38.64 +15:31:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.764 3356298585688310656 099.66139324715 +15.51781526961 13.3108 12.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200570_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200570_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:50.62 +17:03:30.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200571_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200571_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:42.29 +17:12:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200572_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200572_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:45.66 +14:35:32.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200574_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200574_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:51.79 +15:45:28.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 200576_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200576_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200580_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200580_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:59.96 +17:13:50.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200583_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200583_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:49.84 +18:08:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.563 3371118838496744320 099.20775087986 +18.13376271270 13.4389 12.8968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200584_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200584_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200589_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200589_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:53.37 +14:53:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 5.873 3348442785564414976 090.22237169739 +14.89467411197 13.2417 12.2834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200590_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200590_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200591_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200591_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200592_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200592_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:47.77 +13:23:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.387 3343787006656105344 089.94943995237 +13.38691578193 13.3344 12.4578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200594_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200594_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200598_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200598_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200599_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200599_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:10.21 +09:49:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200601_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200601_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200606_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200606_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:09.37 +15:25:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.668 3356858310124916992 096.78888066491 +15.42148867849 13.1779 12.2848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200609_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200609_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:45.90 +14:41:17.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200611_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200611_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:54.62 +15:45:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 4.966 3348652448686763392 090.47806853220 +15.75009089274 13.7138 13.1927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200612_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200612_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:58.18 +10:26:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.293 3341819293158617600 090.74279881579 +10.44415236550 13.5918 12.6443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200613_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200613_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200614_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200614_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:10.85 +13:44:44.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200615_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200615_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:09.72 +13:57:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.592 3346833581577034496 088.04044301436 +13.95989233941 13.7688 13.2035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200616_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200616_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200617_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200617_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:26.47 +10:23:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.009 3341794240611721344 089.86013282122 +10.38678400560 13.2799 12.4249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200618_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200618_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:56.64 +10:15:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.891 3341722634915166080 090.48562133234 +10.25690221994 13.8851 13.3807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200621_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200621_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:33:14.95 +17:55:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.157 3371071211602935680 098.31183692162 +17.91781816822 13.6330 13.2013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200622_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200622_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:15.45 +10:20:57.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 200623_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200623_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:24.26 +15:56:58.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 200625_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200625_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:15.71 +09:56:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200627_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200627_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:42.47 +18:00:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 5.696 3371111244994678400 098.92729980490 +18.01406271266 13.4307 12.6286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200633_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200633_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:23.64 +12:57:12.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
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Considering the candidate 200634_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200634_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200635_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200635_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:46.92 +14:33:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.906 3346976616871654144 088.94637423385 +14.56226522685 13.3919 12.7463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200636_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200636_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:05.28 +14:27:04.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 200638_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200638_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:01.05 +15:01:22.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
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Considering the candidate 200641_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200641_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:28.51 +14:40:23.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 200646_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200646_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:04.85 +13:51:49.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 200647_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200647_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:26.72 +11:01:17.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)
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Considering the candidate 200650_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200650_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200655_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200655_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:51.00 +12:47:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.528 3355326003233356544 099.21253469582 +12.79682615899 13.2400 12.3342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200656_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200656_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:30.76 +16:54:11.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 200660_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200660_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200661_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200661_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:31:08.60 +12:34:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.878 3331255116718177280 097.78599835561 +12.57137676187 13.3170 12.7319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200663_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200663_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:48:26.80 +11:36:15.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 200668_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200668_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:41.05 +16:47:34.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 200669_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200669_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:22.47 +14:30:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200672_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200672_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:29.87 +14:18:29.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 200673_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200673_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:14.25 +16:46:07.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)
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Considering the candidate 200674_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200674_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:37.67 +12:17:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.065 3352202153259675008 099.40710830951 +12.28732284965 13.5700 13.1238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200675_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200675_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200676_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200676_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:39.25 +14:41:34.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 200677_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200677_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:57.87 +16:30:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.885 3369226201028342144 095.49084930419 +16.50105798305 13.2236 12.3003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200678_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200678_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:25.19 +16:41:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.796 3348969176754954496 090.10511161981 +16.69206336924 13.3456 12.8802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200681_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200681_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:40.55 +15:46:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.412 3348804937206620928 088.91889051539 +15.76760940675 13.3626 12.8941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200682_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200682_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 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 200684_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200684_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:24.98 +17:30:51.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 200685_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200685_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:51.87 +12:31:32.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 200686_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200686_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:31:42.96 +11:11:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 5.893 3328000493581306752 097.92881432258 +11.18540110827 13.2845 12.8083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200687_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200687_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:40.67 +10:09:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.124 3327646107239611136 098.91946569345 +10.16410450905 13.0310 12.4233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200688_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200688_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:41.98 +15:47:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 5.827 3348055203416947200 088.42464027590 +15.78465325625 12.9961 12.0151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200691_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200691_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:11.65 +13:17:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.860 3352743181700220416 100.04829620398 +13.28237142627 13.2231 12.6958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200693_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200693_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:41.02 +12:33:23.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 200694_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200694_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:12.40 +15:20:15.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
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Considering the candidate 200695_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200695_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:24.49 +14:24:25.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 200696_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200696_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:50.99 +11:55:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.675 3331908398425863936 092.96247692772 +11.92884037681 13.3306 12.9628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200701_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200701_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:55.14 +12:51:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.478 3346244105904547712 087.47925838724 +12.86072256822 13.5209 12.8174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200702_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200702_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:18:55.73 +14:18:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 5.782 3344652734623361280 094.73200870765 +14.30923901219 13.3879 12.9368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200704_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200704_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:24:36.81 +13:56:47.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
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Considering the candidate 200705_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200705_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:12.96 +15:28:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.683 3348723916943902464 089.55390253484 +15.47986861112 12.9930 12.0903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200707_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200707_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:58.28 +17:40:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.283 3359405260091107712 100.49373375074 +17.66564264759 13.7133 12.8687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200709_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200709_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:06.68 +15:32:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.739 3347282732077063936 088.77811283212 +15.53870650037 13.3331 12.8121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200711_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200711_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:58.28 +15:26:17.8 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 200717_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200717_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200720_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200720_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:54.71 +13:07:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.761 3355364554859351680 099.47766021176 +13.12849639098 13.2502 12.7300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200721_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200721_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:36.75 +11:00:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200724_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200724_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:33:38.72 +18:00:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.983 3371078186628115072 098.41154734941 +18.00690866914 13.2750 12.7495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200726_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200726_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200727_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200727_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:14.79 +15:57:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.884 3348867849887081728 089.81213057091 +15.96460605318 13.4483 13.1512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200728_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200728_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:36.66 +15:10:26.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 200729_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200729_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:55.70 +15:51:00.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 200730_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200730_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:18.23 +12:59:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 5.563 3346330859948569472 088.07603923236 +12.98256789099 13.0304 12.2583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200733_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200733_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:36.14 +10:15:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.379 3329935187370341504 092.65063014769 +10.25417316896 13.1642 12.6042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200734_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200734_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:47.80 +14:01:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.875 3346661297550515712 087.69898674083 +14.02943293892 13.2527 12.6974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200735_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200735_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:38.90 +10:08:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200736_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200736_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:26.29 +12:32:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.227 3355235018645886464 098.60956251724 +12.54490924979 13.0812 12.6075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200740_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200740_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200741_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200741_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:33.97 +17:02:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 5.537 3369494615005603328 097.39132749198 +17.04367013673 12.9638 12.1381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200744_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200744_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:59.09 +14:43:11.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 200745_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200745_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:01.55 +14:25:00.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)
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Considering the candidate 200747_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200747_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:11.47 +17:16:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 5.186 3358967517023842432 099.04709528123 +17.27149991095 13.2052 12.3505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200748_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200748_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:22.25 +13:13:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.451 3355412452335116288 098.59259090968 +13.21879583731 12.8025 11.9724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200756_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200756_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:23.48 +18:09:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.730 3370577191581233536 096.59810207859 +18.15685003792 13.0528 12.5489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200757_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200757_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:54.59 +16:12:53.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 200760_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200760_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:01.21 +15:56:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.670 3348292908385419392 087.25500421569 +15.94636983274 12.9733 12.4627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200761_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200761_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:29.96 +16:07:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.821 3369142874366218880 095.62489979384 +16.12782876583 13.0531 12.2009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200762_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200762_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:28.56 +17:53:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.009 3350416408935551360 089.11880635332 +17.88587086455 12.8342 11.9671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200763_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200763_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:26.37 +17:51:35.8 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 200764_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200764_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:30:10.18 +15:59:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 5.214 3357277219757852928 097.54247058600 +15.99344144549 13.1387 12.7613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200765_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200765_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:33.60 +10:55:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.443 3327790482561445120 099.63954028936 +10.92201786497 13.2051 12.7392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200767_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200767_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200768_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200768_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:56.95 +17:17:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.276 3350127718413686400 090.23726801113 +17.28697909644 13.0538 12.5377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200771_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200771_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:39:04.55 +13:02:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.350 3352362613238032896 099.76842513863 +13.03571450182 13.2186 12.8475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200773_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200773_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:56.30 +13:42:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.286 3343858131313951872 089.48522629792 +13.69989014071 13.2025 12.7785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200776_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200776_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:11.40 +17:08:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.155 3358906219250904832 099.54767271869 +17.13480225109 13.0151 12.2435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200777_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200777_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:04.03 +17:33:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.496 3359036477018822400 100.01702250302 +17.55869300511 12.8368 11.9846 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 200778_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200778_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:49.61 +15:40:49.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 200779_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200779_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:25.37 +10:51:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.819 3336840086031134848 087.35573390163 +10.85255037733 13.1472 12.6575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200780_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200780_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:30:27.18 +17:19:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.870 3369526535206375808 097.61303605468 +17.32449352883 13.2195 12.9856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200782_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200782_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:46.98 +15:00:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.661 3348503945894885888 089.69562337098 +15.00432223628 13.1156 12.3351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200784_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200784_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:56.44 +13:58:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 5.427 3344587927857524736 093.73459045725 +13.97962793871 12.9646 12.1577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200786_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200786_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200788_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200788_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:48.78 +17:56:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.268 3359474628103142784 100.20312566732 +17.94515254686 13.0081 12.3381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200789_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200789_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:34.08 +14:49:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.397 3347148282420493824 087.64192728517 +14.81766921348 12.9481 12.4323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200792_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200792_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:03.33 +10:47:55.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)
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Considering the candidate 200793_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200793_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:03.88 +15:28:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.810 3348723848224440448 089.51616739585 +15.47324720824 12.5929 11.6977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200794_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200794_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:06.29 +10:08:48.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 200795_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200795_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200799_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200799_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:14.20 +14:51:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 5.068 3356906581257897344 098.80894290809 +14.85269221659 12.9511 12.3659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200800_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200800_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:24.61 +17:04:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.978 3358801628206452736 100.10263151082 +17.07073178886 12.8977 12.3066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200804_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200804_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:59.96 +15:44:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.643 3348065790514994304 088.24981372046 +15.74126609066 13.0203 12.7619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200805_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 200805_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 200806_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200806_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:26.59 +12:41:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200809_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200809_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:48.82 +18:17:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.647 3373528967983878912 092.70327976722 +18.29677016067 12.8483 12.3800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200814_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200814_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:33.08 +15:12:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 4.643 3345006433769473152 093.88755384839 +15.20812765193 13.0634 12.4369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200816_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200816_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:11.22 +14:32:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.344 3348426907065674496 090.04698014769 +14.53414740740 12.8398 12.3311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200818_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200818_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:42.70 +10:29:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200826_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200826_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:51.94 +15:59:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.497 3358580317132401536 099.71605556376 +15.99004067513 12.6742 11.9258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200828_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200828_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:53.58 +15:42:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.585 3348095099371591168 087.47315297195 +15.70692516451 12.6438 12.1920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200829_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200829_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:49.84 +11:40:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.078 3342957459492164480 089.20774551914 +11.67856443397 12.7312 12.2653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200831_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200831_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:26.35 +11:35:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 4.689 3331837033249603712 093.36004479014 +11.59155469199 12.2866 11.2188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200832_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200832_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:13.78 +12:38:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.495 3344028280737452160 092.80757431934 +12.64692750551 13.0518 12.5275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200833_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200833_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:41.16 +15:50:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.168 3348111488966539008 087.92144800561 +15.83784317950 12.2328 11.4364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200837_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200837_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:12.70 +15:24:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 3.397 3348722435181321984 089.30298874626 +15.40647573700 13.0135 12.5762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200838_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200838_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:21.15 +10:11:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.021 3327655040771108736 098.58813851330 +10.19118888818 13.1780 12.7292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200839_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200839_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:54.61 +15:09:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.462 3345003100874876032 093.72754716974 +15.16495509563 12.4389 11.5841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200840_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200840_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:32.27 +15:40:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.856 3348798095319160192 088.88454286666 +15.66601454268 12.6132 12.1562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200841_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200841_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:51.50 +10:51:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200846_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200846_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:09.02 +15:26:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.731 3347286820886044032 088.53725205079 +15.43316977211 12.5872 12.0464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200847_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200847_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:47.02 +12:13:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 4.464 3343201757231045248 087.69588515421 +12.21553816911 12.5120 11.9390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200848_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200848_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:11.25 +16:10:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 5.753 3345887623619012736 093.54680330667 +16.16512556569 12.5646 11.7946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200849_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200849_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:05:19.24 +14:12:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.685 3345175827279012224 091.33039300686 +14.21027805006 13.1116 12.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200851_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200851_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:27.48 +17:54:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200852_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200852_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:19.61 +14:13:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.603 3356440113449222528 097.08143008752 +14.21572250391 11.8154 10.6198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200853_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200853_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:52.20 +15:55:29.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
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Considering the candidate 200854_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200854_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:23.42 +17:37:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 5.561 3373477973834339328 092.09763390040 +17.63173370806 12.1002 11.0310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200855_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200855_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:05.34 +14:02:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.740 3347025274558597504 087.77212076487 +14.04549476456 12.6176 12.1463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200856_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200856_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:02.55 +15:00:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.764 3347202158489229696 089.01028924039 +15.00045035307 12.4937 11.7723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200857_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200857_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:18:11.38 +12:49:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 4.454 3332028588791330688 094.54731863566 +12.82807196706 12.8564 12.5114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200858_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200858_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:05:56.69 +12:59:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 4.027 3342776795986519680 091.48619042234 +12.98424270358 12.6805 12.2078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200860_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200860_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:53.72 +17:55:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.406 3350244434147448960 089.72428424972 +17.91996228641 12.7755 12.2702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200861_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200861_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:14.07 +13:40:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 4.122 3355785358575117696 100.05818685553 +13.68218700450 12.6991 12.4615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200862_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200862_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:17.64 +16:09:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.309 3368967334760146560 096.32332009104 +16.16086869320 12.2561 11.3997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200864_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200864_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:56.50 +14:43:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.119 3346991838232847744 089.23554296276 +14.71527762171 12.2346 11.4939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200865_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200865_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:51.40 +15:52:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 5.262 3368935204108493184 095.96416624453 +15.87867727057 12.6190 12.0750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200867_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200867_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:42.89 +13:25:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.634 3343750069937229696 089.42874704002 +13.42896355669 12.4048 11.7110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200868_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200868_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:36.81 +17:53:12.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)
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Considering the candidate 200869_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200869_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:29.63 +14:45:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 5.038 3344837413921531520 093.87339326052 +14.76299093228 12.2147 11.3601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200872_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200872_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:14.17 +13:23:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 5.077 3343611836409867776 090.55934277124 +13.39203724678 12.5807 12.3331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200875_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200875_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:41.63 +16:57:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 4.526 3349355650793620736 090.42327903366 +16.96453223120 12.3827 12.0132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200877_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200877_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:15.33 +14:22:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.534 3356115280782032000 098.56346443590 +14.37624135499 12.4568 12.0331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200878_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200878_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:42.69 +12:40:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.965 3343278173290186752 088.67786817265 +12.67637075116 12.2889 11.7990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200879_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200879_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:44.21 +16:10:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 4.675 3348886434206484480 090.43444357496 +16.16816562750 12.4774 12.1700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200881_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200881_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:11.76 +15:26:19.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)
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Considering the candidate 200883_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200883_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:59.30 +17:48:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.894 3369781724979663744 096.74716619232 +17.80617132422 12.3751 12.0085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200893_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200893_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:44.87 +16:35:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 3.471 3358683495127303040 099.68713909596 +16.58366262296 12.2463 11.4557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200894_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200894_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:40.43 +11:48:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 3.697 3337148529106292224 087.41806972761 +11.80910156059 12.0512 11.2523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200896_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200896_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:48.83 +16:28:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.852 3349697878087629184 089.20341727050 +16.47918098784 12.1159 11.6774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200898_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200898_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:15.64 +16:47:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.550 3349766387108428544 089.06506399157 +16.79401874301 11.7978 10.9640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200900_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200900_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:30:28.13 +16:59:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 4.944 3369479565442237312 097.61689195553 +16.99785494787 12.1899 11.9093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200901_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200901_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:10.88 +13:33:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.822 3346441880559578368 087.79522024758 +13.56041623763 11.8536 11.2904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200904_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200904_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:47.26 +13:09:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 2.491 3355399391336685696 098.69663990043 +13.16233481249 11.7429 11.2973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200905_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200905_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:18.86 +11:30:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 2.134 3328081921862272384 098.82825432242 +11.50141915759 11.6717 11.2658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200906_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200906_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:27.38 +12:40:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 2.672 3343442752139818624 089.86457056348 +12.67020789632 11.4521 10.9434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200907_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200907_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:05.16 +17:19:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200908_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200908_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:47.80 +09:57:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 2.620 3341687145604221568 090.19884653379 +09.96017735157 11.1479 10.2501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200909_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200909_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:19:23.90 +17:39:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.797 3370664224799960960 094.84945476925 +17.64906359742 11.1260 10.2621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200914_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200914_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:41.77 +16:32:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 3.030 3369541211110732672 096.42382454315 +16.54082334187 10.9869 10.2679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200915_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200915_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:25.71 +16:03:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 3.093 3357845053090488832 100.35714121559 +16.06408544540 11.0387 10.6139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200916_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200916_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:26.91 +17:16:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 2.440 3349986323792979328 088.86212951416 +17.27215543188 11.0935 10.8277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200917_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200917_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:17.85 +15:55:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 3.310 3345875838228836480 093.32432743061 +15.91797045444 11.0973 10.7666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200921_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 200921_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:18.65 +14:00:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.11, MAG_FAINT_SEARCH_LIMIT=10.09)GAIADR2_OUTPUT=# 0.852 3345194347178716800 092.07770715289 +14.00376444567 8.3071 7.1898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201017_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201017_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:15.41 +15:33:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.16, MAG_FAINT_SEARCH_LIMIT=11.14)GAIADR2_OUTPUT=# 2.009 3345750115942949120 092.81452392098 +15.56272641147 10.3958 9.9883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201023_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201023_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:18.68 +13:59:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 2.857 3345194347176271872 092.07802470555 +13.98856167066 10.5449 10.4762 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 201061_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201061_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:35.81 +11:51:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.33, MAG_FAINT_SEARCH_LIMIT=11.31)GAIADR2_OUTPUT=# 2.086 3352113986172044928 099.14889968554 +11.85436674720 10.7155 10.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201065_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201065_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:25.30 +15:43:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 1.203 3357096216952323968 098.85533171442 +15.71842612673 10.4561 9.7252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201108_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201108_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:05.14 +15:12:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 2.891 3348478657131124480 090.52162924754 +15.19941809654 10.6687 9.8662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201188_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201188_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:59.99 +18:04:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 2.595 3350286009430416896 090.75017501953 +18.06644822458 11.2410 11.0507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201222_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201222_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:51.81 +14:13:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201236_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201236_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:44.09 +16:56:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 2.879 3349354791800163072 090.43370513177 +16.93625582270 11.1866 10.4013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201264_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201264_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:20:52.45 +17:20:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 2.451 3370453148628289792 095.21855338735 +17.34845814795 11.3304 10.8012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201278_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201278_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:25.58 +13:44:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201301_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201301_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:43.89 +16:47:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 2.416 3369392296004628736 096.93299990475 +16.78342297646 10.8171 9.7201 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 201306_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201306_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:22.73 +14:04:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 3.189 3343905955772961152 089.84487003571 +14.08010042817 11.4251 10.6755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201318_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201318_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:14.39 +12:08:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 2.106 3343033188355163520 088.81019156062 +12.13335025078 11.6539 11.0987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201322_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201322_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:25.18 +13:26:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 0.928 3343604281566297728 090.35498295526 +13.44963933601 11.8865 11.1545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201344_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201344_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:44.78 +11:17:02.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 201354_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201354_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:53.91 +17:16:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 4.225 3349388949677927296 090.97458706794 +17.27949370533 11.7662 11.4565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201356_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201356_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:26.78 +15:43:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 3.176 3348086264620416256 087.86177490020 +15.72166490026 12.0083 11.6320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201358_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201358_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:27.10 +14:32:55.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)
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Considering the candidate 201362_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201362_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:41.96 +12:49:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.852 3355282430785145216 098.17458912287 +12.82362345476 11.7401 11.3027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201366_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201366_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:33.30 +16:49:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 4.678 3349206327668085504 091.63881200775 +16.81747961446 11.6869 11.0212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201389_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201389_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:19.07 +17:40:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 3.094 3350026528984261632 089.07931686384 +17.66681788967 11.5881 10.9490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201450_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201450_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:01.73 +10:51:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 4.572 3336839501915593600 087.25715516966 +10.85736991660 11.8198 11.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201459_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201459_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:59.36 +16:45:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 3.537 3349167015830923776 092.49717291038 +16.75683508035 11.8807 11.3393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201481_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201481_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:48.73 +10:25:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 5.104 3336752464402088576 087.95297007775 +10.42713959719 12.0271 11.3473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201493_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201493_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:54.78 +17:41:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 4.097 3369776987634402176 096.72833246704 +17.69719812288 11.9736 11.4653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201496_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201496_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:24:33.79 +16:49:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.698 3369616179760034304 096.14071357557 +16.83039313453 11.8023 10.9960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201515_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201515_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:53.29 +17:47:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.864 3369792483876730880 097.22206187216 +17.79278797109 11.8663 11.0490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201569_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201569_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:52.96 +16:26:13.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 201583_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201583_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:26.31 +13:30:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.362 3332545080078277120 095.35960441075 +13.51095521187 11.9295 11.0255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201609_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201609_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:50.90 +17:12:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.371 3358825503925493760 100.46173302454 +17.20315310497 12.3347 11.9111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201610_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201610_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:50.43 +16:42:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 5.657 3349145300476276608 092.20999595535 +16.70776690786 12.2595 11.5481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201619_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201619_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:34.12 +16:48:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 5.485 3349206117214115328 091.64227933264 +16.81098027263 11.6160 10.4880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201621_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201621_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:33.21 +17:31:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 4.234 3359024996567565824 100.13798012589 +17.53080245731 12.2270 11.4894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201626_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201626_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:45.59 +13:50:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.833 3346642747589641472 087.68980554282 +13.83755671432 12.1733 11.6438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201682_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201682_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:17.61 +11:05:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 4.999 3342069397692976768 089.57359010533 +11.09829426935 12.5386 11.9642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201684_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201684_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:19:35.88 +16:11:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 4.171 3369111125966694272 094.89945935501 +16.18923088560 12.2352 11.7144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201687_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201687_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:17.23 +16:32:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 4.456 3348917083093093632 090.32177078968 +16.53909581331 12.4054 12.0390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201707_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201707_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:27.02 +17:10:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.916 3370388449239528448 095.61265851950 +17.17588643624 12.1563 11.7205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201732_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201732_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:17.35 +10:01:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201734_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201734_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:10.06 +12:00:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 2.714 3343127810780887168 088.29206491820 +12.00170468539 12.6041 12.1842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201737_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201737_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:33:20.20 +18:02:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 4.979 3371081897479858048 098.33438876504 +18.04146638911 11.8644 10.8017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201741_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201741_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:32.35 +13:10:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 4.639 3346360546762559104 088.38504790172 +13.16795797092 12.3235 11.7916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201743_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201743_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:10.66 +14:28:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 4.770 3344825735905847168 093.54439435012 +14.47300843745 12.3357 11.8265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201792_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201792_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:17.04 +15:47:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.462 3348803111840941696 088.82124704033 +15.79662379989 12.3597 11.5905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201822_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201822_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:17.49 +10:29:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.024 3336018437310464640 088.82277253038 +10.49369389243 12.4558 11.9961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201824_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201824_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:50.69 +15:25:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 5.088 3347286649087380736 088.46104249624 +15.42429021899 12.7016 12.3284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201832_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201832_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:20.87 +15:41:23.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)
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Considering the candidate 201833_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201833_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:20.03 +11:40:04.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201841_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201841_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:05:58.71 +15:28:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.629 3345591747613893376 091.49468762610 +15.47852124743 12.1418 11.2297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201860_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201860_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:32.83 +17:28:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 4.803 3359023042361110272 100.13650757046 +17.46780481902 12.7382 12.1493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201867_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201867_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:57.27 +15:39:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 5.060 3357232693834767360 097.48871068355 +15.65001346320 12.4718 12.0006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201881_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201881_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:30.39 +11:22:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 4.375 3342842556227533696 089.12709839198 +11.37126581374 12.6524 12.1520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201883_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201883_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:32.09 +16:35:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.071 3349712236160778112 089.13357613302 +16.58379294168 12.6162 12.0249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201887_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201887_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:30.55 +16:25:09.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 201894_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201894_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:58.34 +17:17:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 5.204 3369657965500857984 096.49314948059 +17.28369462775 12.1505 11.1256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201941_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201941_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:24.08 +14:06:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 4.457 3343906063148807040 089.85029497556 +14.10465139972 12.5161 11.9505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201946_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201946_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:44.92 +15:20:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 5.446 3368805461733609216 095.68678006227 +15.33245045022 13.4323 12.3071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201962_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201962_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:04.29 +09:51:55.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)
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Considering the candidate 201973_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201973_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:40.15 +12:12:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201994_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201994_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:31:02.40 +16:57:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 4.588 3369454796368516480 097.75982259933 +16.95657018374 12.5728 12.0889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201997_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201997_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:05.54 +16:43:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 5.339 3349720589874563968 089.27344231483 +16.71714082128 12.7106 12.1629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201999_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 201999_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:28.00 +12:53:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.769 3346325057449619840 088.11692928040 +12.88428363636 12.8257 12.4507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202000_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202000_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:41.94 +10:55:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.660 3342013391319536640 089.42479045164 +10.91659520686 12.8175 12.2907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202017_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202017_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:45.87 +12:05:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202027_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202027_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:09.30 +13:52:43.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202036_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202036_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:08.45 +15:03:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.413 3348484601365627776 090.03541349476 +15.06454031990 12.7473 12.3633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202044_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202044_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:33.80 +16:11:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 4.227 3346112954783949312 092.64047008736 +16.18848996232 12.5471 11.6939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202046_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202046_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:48:14.49 +15:36:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.483 3348189382493112320 087.05942919569 +15.60786860225 12.6739 12.0459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202049_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202049_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:37.56 +15:34:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 5.806 3348606131759642112 091.15654701349 +15.57666566456 12.6935 12.2511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202058_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202058_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:15.04 +17:30:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 4.078 3369720912541847296 097.31247712788 +17.50477058305 12.6315 12.0607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202064_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202064_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:06.23 +15:18:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.464 3348550640782766848 089.77619038632 +15.30647096774 12.5791 11.8219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202075_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202075_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:06.50 +12:58:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.546 3344089887749562624 093.52687633102 +12.96714694997 12.6271 11.8167 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 202086_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202086_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:08.27 +16:08:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.118 3346106628293286528 092.53418164039 +16.13407556003 12.8702 12.3518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202092_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202092_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:37.98 +14:27:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.507 3355976123841683072 100.15861974061 +14.45148491578 12.7423 12.4904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202093_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202093_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:20.95 +13:38:22.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202100_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202100_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:11.25 +13:28:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 5.402 3344188117941795328 093.29695687676 +13.48089033685 12.4364 11.5593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202115_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202115_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:33.22 +17:33:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 5.231 3373251684895191168 093.13838267387 +17.56485293110 12.7419 12.2267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202130_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202130_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:17.70 +14:55:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.067 3345543304681287936 091.07364541085 +14.92006827721 13.0594 12.4100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202132_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202132_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:43.32 +18:12:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.579 3370569563719615104 096.93057530962 +18.20300784835 12.5903 11.9228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202134_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202134_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:39.07 +18:04:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 5.071 3371264897445816704 098.16268778843 +18.07215031061 12.6055 12.2284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202140_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202140_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:44.15 +12:53:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.343 3332225637592956544 095.43382461227 +12.88902277851 12.5884 12.0617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202149_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202149_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202175_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202175_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:00.62 +11:19:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.211 3330128735775582464 093.50223588631 +11.32388105680 12.9329 12.4245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202187_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202187_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:19.73 +13:11:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.032 3346404767743098880 087.33200740963 +13.18469935554 12.5569 11.7444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202210_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202210_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:04.29 +17:22:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 5.164 3359019297149615744 100.26791964743 +17.37403841393 12.8089 12.0202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202216_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202216_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202231_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202231_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:35.89 +18:02:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.979 3369815225728089216 096.89934601707 +18.03979615527 12.8265 12.0704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202234_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202234_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:48.54 +13:31:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.476 3344168640269409920 093.20203572497 +13.51754871453 13.0075 12.6339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202244_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202244_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:00.74 +12:28:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.750 3343257557447133184 089.00299742522 +12.46643385548 13.0756 12.8794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202247_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202247_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:22.86 +13:08:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 5.133 3346368213280601088 088.09539984189 +13.13538718664 12.7517 12.0042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202248_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202248_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:19:06.30 +14:39:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.890 3344737946774121728 094.77591751462 +14.64990260514 12.5819 11.7497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202254_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202254_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:27.51 +14:46:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.122 3344837486936182912 093.86443664937 +14.77100567174 12.9905 12.5320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202258_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202258_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:51.04 +13:51:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.072 3346795510987201920 088.71351314086 +13.85452006185 12.9355 12.5218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202296_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202296_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:09.90 +18:03:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.981 3373410289448225920 093.29117179049 +18.05539678744 12.9907 12.4924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202302_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202302_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:52.77 +17:32:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.133 3370438756195767168 095.71992116925 +17.54374160170 12.9709 12.5361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202304_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202304_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:23.10 +15:49:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.347 3348064519204708992 088.09616932128 +15.81598930374 12.8109 12.2654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202305_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202305_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:19.98 +14:26:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 5.762 3345279181372314624 091.58377857882 +14.44006689857 13.1161 12.6793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202311_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202311_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202314_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202314_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:45.62 +16:34:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.314 3358683499426096384 099.69014868992 +16.57008071522 12.9299 12.4047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202315_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202315_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:06.34 +17:09:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.949 3349760928207104000 089.52620984621 +17.15442108860 12.6940 11.7654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202326_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202326_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:19.35 +13:11:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.999 3344249763610589184 092.58101034558 +13.19807976003 13.0992 12.5818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202335_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202335_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:54.60 +11:04:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 5.419 3342057577942876672 088.97765909997 +11.08128069186 12.9648 12.4305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202353_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202353_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:22.80 +14:22:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202361_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202361_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:23.40 +13:50:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.719 3344429052725516928 092.59752528287 +13.83418932603 11.2198 9.8179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202386_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202386_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:09.38 +13:38:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.340 3346765274417578880 088.53885976439 +13.63239738016 12.9168 12.1783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202390_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202390_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202394_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202394_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:42.54 +12:17:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 5.810 3343195091441390464 088.17746570654 +12.29476105520 12.8012 11.9325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202407_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202407_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:20:43.02 +18:02:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.878 3370702943926205312 095.17934314625 +18.04181447075 12.5599 11.6093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202409_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202409_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:07:30.51 +11:00:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 5.796 3330254762997242112 091.87675871697 +11.01165296275 12.6619 11.8391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202413_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202413_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:34.57 +11:46:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.612 3331835865018398592 093.64382764862 +11.77673314445 12.9518 12.5412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202416_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202416_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:37.43 +18:05:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.630 3370598730838491264 095.90613188866 +18.09369680463 12.9520 12.4070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202417_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202417_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202420_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202420_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:45.34 +15:33:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.885 3345044985395863680 094.18862643768 +15.55547266755 12.7012 11.8365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202425_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202425_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:21.12 +14:14:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.538 3356097276279530752 098.83816659692 +14.24414173464 13.4308 12.5562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202430_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202430_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:49.88 +13:38:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.951 3343853144854246784 089.70735625011 +13.64428855046 13.1372 12.5806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202433_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202433_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:03.60 +15:41:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.457 3348763976098955776 089.51521611652 +15.69736277212 13.0586 12.5587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202437_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202437_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:19:17.69 +17:44:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.785 3370668519767227264 094.82390688747 +17.74726520699 13.0272 12.1707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202439_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202439_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:18:39.55 +17:35:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.198 3370290665722797824 094.66447383406 +17.59444925488 13.0097 12.5044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202440_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202440_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:12.25 +11:14:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.046 3342870529353525632 088.30102247681 +11.24718181503 13.0267 12.3759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202442_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202442_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:07:14.78 +16:34:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 5.762 3349058198540181760 091.81163502854 +16.56617794186 12.8725 12.2819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202457_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202457_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:22.05 +10:45:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 5.506 3330220098320870016 091.59153720188 +10.75272917484 13.0258 12.7165 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 202463_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202463_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:46.85 +17:35:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.457 3350208326359314176 089.44609958617 +17.59735799575 13.1928 12.6883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202467_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202467_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:59.99 +14:14:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202480_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202480_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:25.40 +16:58:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.926 3349740724680896128 089.85596284808 +16.97452630478 12.5659 11.7051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202488_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202488_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:34.27 +13:26:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202489_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202489_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:34.20 +15:33:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.575 3345969056199793024 091.64250816233 +15.55045144262 12.5929 11.6569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202496_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202496_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:49.44 +17:20:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.544 3349815147874197248 089.45580863539 +17.34113746329 13.1921 12.6949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202499_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202499_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:07:26.07 +16:10:13.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 202500_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202500_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:43.22 +15:24:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202501_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202501_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:18.94 +10:02:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.550 3329889076601331584 093.07876972070 +10.03990965761 12.9442 12.1558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202502_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202502_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:03.33 +13:39:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.767 3332364317793274368 096.51348785808 +13.66183163531 12.3351 11.2653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202503_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202503_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:57.34 +15:37:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.987 3345805740064507776 093.73884263204 +15.63167212358 13.1680 12.7977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202505_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202505_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:52.07 +18:15:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.037 3350312947466883712 090.96696986183 +18.25223973825 12.7086 11.6825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202507_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202507_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:24.80 +17:53:06.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202516_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202516_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:05:30.93 +16:17:57.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 202524_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202524_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:37.55 +13:51:44.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 202558_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202558_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:38.60 +15:45:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 5.394 3369068799066487936 094.41054549919 +15.76138858278 13.1102 12.6108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202559_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202559_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:27.16 +14:25:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 5.143 3347108665642267136 087.36308326166 +14.42501805852 12.8995 12.3044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202561_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202561_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:21.70 +13:07:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.017 3344245777880783360 092.34027427484 +13.12439119931 13.2273 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202571_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202571_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202586_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202586_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:15.91 +13:14:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 5.484 3344111018988845440 094.06606377346 +13.23196502846 13.3168 12.7369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202590_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202590_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:33.14 +17:47:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.866 3373319682817256576 092.63744702108 +17.78734851698 13.4521 12.9017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202613_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202613_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:15.79 +09:57:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 5.413 3336640176776475136 087.56561476189 +09.95686772871 13.0296 12.4604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202617_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202617_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:57.72 +17:51:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.473 3350418981618210304 088.99048454188 +17.85720204125 12.9885 12.4559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202622_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202622_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:05.02 +10:00:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202625_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202625_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:43.64 +12:19:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.607 3342641384257644416 090.68148577155 +12.32261880052 13.3530 12.9573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202646_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202646_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:12.15 +15:48:01.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 202661_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202661_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:29.55 +15:49:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 5.436 3357250767057119104 097.37309398805 +15.82693469515 13.2807 12.8444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202665_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202665_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:24:40.67 +17:23:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 4.113 3369668548300338176 096.16947898442 +17.38791309686 12.8737 11.9815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202673_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202673_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:20.28 +13:08:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.974 3346368277701929728 088.08453618645 +13.14847999423 12.8927 12.4001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202677_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202677_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:08.45 +10:34:30.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202680_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202680_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:28.05 +16:25:10.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 202688_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202688_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:19.33 +17:13:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.979 3369691221428831872 097.08045195488 +17.23070353826 13.2581 12.9854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202694_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202694_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:24.18 +18:05:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.844 3370566398327364352 096.85066233207 +18.09629582934 13.1704 12.7036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202698_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202698_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 202700_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202700_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:04.06 +11:53:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.286 3352115047023177088 099.26648689796 +11.88543995926 13.1043 12.1401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202709_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202709_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:16.39 +17:30:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.145 3369720946901581056 097.31823966737 +17.51023825738 13.1093 12.7794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202713_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202713_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202719_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202719_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:40.01 +11:53:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.621 3342932681823339520 088.66668105157 +11.89135554383 13.1100 12.2864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202723_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202723_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:12.74 +14:41:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.193 3346990880459737856 089.30363649453 +14.69846597807 13.4641 13.2528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202733_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202733_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:41.49 +15:32:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202740_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202740_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:39.85 +16:37:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.882 3348953783592272128 089.66634880272 +16.61765141382 13.5213 13.1340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202756_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202756_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:06.00 +16:07:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.141 3369283581793126528 097.02506493190 +16.12232338273 13.0129 12.1988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202764_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202764_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202767_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202767_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:17.08 +15:54:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.419 3345875735149626496 093.32103278618 +15.90202815244 13.3038 12.9097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202780_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202780_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202782_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202782_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:33:49.38 +18:00:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.007 3371078053487168128 098.45570931479 +18.00055422262 13.2296 12.7323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202785_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202785_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:43.86 +16:41:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202791_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202791_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:27.84 +17:09:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.408 3370223286275686912 093.36551705681 +17.16326493666 13.3028 12.7817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202795_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202795_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:53.52 +17:20:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.260 3370266197291202560 093.97277893926 +17.33905411562 12.7462 11.8069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202798_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202798_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:41.28 +13:46:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.606 3346650100573394944 087.42187520447 +13.77192078285 13.1659 12.6057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202809_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202809_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:52.96 +13:12:49.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 202810_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202810_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202817_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202817_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:57.56 +11:08:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.673 3330119179469646848 093.23963625886 +11.13874425129 13.0992 12.2623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202822_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202822_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202823_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202823_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202828_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202828_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:19.39 +15:25:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.818 3347983116686371968 087.33066232400 +15.42047194750 13.2589 12.9414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202829_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202829_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:52.81 +14:11:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.612 3346857289796673536 088.72123456578 +14.19383800812 13.1792 12.6928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202836_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202836_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:25.89 +16:37:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 5.249 3348967527487529984 090.10796848440 +16.61973906657 13.4662 12.9271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202839_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202839_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202848_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202848_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:43.86 +16:12:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.658 3358601482731005312 100.18292939804 +16.20779895812 13.4165 13.0768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202851_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202851_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:07:52.85 +14:21:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.315 3345268697353714688 091.97024192916 +14.36113502853 13.1894 12.6523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202852_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202852_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:23.23 +15:56:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.533 3348119322987332480 088.09684072008 +15.94863088749 12.9684 12.1466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202856_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202856_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202881_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202881_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:08.60 +17:32:28.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 202902_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202902_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202908_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202908_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202913_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202913_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:56.05 +15:17:01.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 202915_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202915_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:46.03 +17:35:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202922_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202922_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:05.20 +17:47:57.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
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Considering the candidate 202923_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202923_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:17.17 +14:34:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.014 3345249765138904064 092.32132783419 +14.56862277810 13.4202 12.8205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202930_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202930_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:39:11.67 +16:28:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.561 3358670030408653952 099.79873430757 +16.47823742762 13.1420 12.4792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202933_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202933_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:17.32 +14:27:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.097 3347065819049420544 088.57221551710 +14.46150149677 13.3778 12.9818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202941_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202941_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:56.51 +18:09:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.108 3370707861667708544 095.48502870894 +18.15088560933 13.2770 12.2382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202945_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202945_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202946_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202946_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:04.11 +09:55:17.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202947_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202947_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:19.79 +14:39:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.619 3345254163187076992 092.58222150890 +14.65015039078 13.5059 13.0642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202949_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202949_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:36.51 +10:30:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202952_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202952_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202953_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 202953_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 202962_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202962_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:32.73 +11:02:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.148 3342057165623036800 088.88687714913 +11.03240769550 13.3639 12.4754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202963_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202963_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:09.64 +12:56:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.994 3346329214977679232 088.04014277091 +12.93847411677 13.1262 12.3577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202975_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202975_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:55.71 +15:29:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 5.783 3345747916923197056 092.73215668122 +15.49231064196 13.3083 12.7671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202978_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202978_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 202982_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202982_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:38.07 +14:13:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.790 3344475507091417088 092.65872944011 +14.22806206946 13.4306 12.8439 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 202985_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202985_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:00.86 +16:09:34.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202988_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202988_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:53.08 +17:36:46.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 202989_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202989_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:17.07 +12:54:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202990_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202990_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:38.62 +14:46:41.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 202992_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202992_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:13.53 +15:43:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.387 3348792292822869248 089.05633156261 +15.73200422078 13.3905 12.8816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202999_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 202999_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:07:08.57 +14:04:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.555 3345117033468990464 091.78578940095 +14.06787566094 13.4199 12.9088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203005_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203005_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203006_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203006_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:14.06 +12:48:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 5.593 3332062226974934016 093.80848461812 +12.80225490251 13.4990 13.0291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203015_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203015_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:32.57 +15:59:28.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 203029_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203029_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:58.12 +11:31:05.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 203031_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203031_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203035_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203035_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:21.81 +17:27:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203040_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203040_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:00.36 +14:23:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.585 3347073103313554816 088.00052194638 +14.39713257143 13.5401 13.1927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203042_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203042_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203048_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203048_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:48.52 +12:49:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.336 3344072467362456960 093.70196302565 +12.82783661078 13.4893 13.1232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203050_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203050_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203053_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203053_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:44.29 +18:06:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.201 3370517538778148736 095.68467336499 +18.10336616559 13.3287 12.8092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203064_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203064_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:45.54 +16:35:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.540 3348952924598815488 089.68976818892 +16.58873912473 12.9994 12.0436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203066_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203066_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:28.48 +17:28:05.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 203069_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203069_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:59.21 +13:01:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.778 3343712583462968448 088.99626854998 +13.02953666856 13.2761 12.7180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203072_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203072_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:43.02 +17:35:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.601 3350164826930635264 090.42881118218 +17.58981371026 13.3657 12.7481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203073_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203073_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203074_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203074_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:12.27 +15:29:04.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 203075_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203075_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:03.55 +13:39:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.107 3332364141695350912 096.51479192999 +13.65224819165 13.0188 12.1662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203077_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203077_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:29.64 +15:06:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203079_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203079_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:23.25 +14:59:09.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 203081_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203081_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203084_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203084_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:48:39.66 +10:58:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 3.929 3337033462639557760 087.16493205109 +10.98200966142 13.5477 12.9816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203104_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203104_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:01.30 +12:54:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.793 3332079887880225920 094.25486750302 +12.91422536403 13.6903 13.1067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203114_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203114_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:00.80 +13:55:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.520 3355696259473513472 098.00353090324 +13.92792591042 13.4473 12.9059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203123_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203123_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:09.00 +15:06:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203125_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203125_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:57.53 +09:49:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203126_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203126_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:41.84 +11:46:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.409 3343091393751973376 088.17414016315 +11.77828722280 13.2729 12.6874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203132_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203132_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:46.06 +17:15:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.662 3349798444741963648 088.94184217360 +17.25265199484 13.3446 12.4932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203133_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203133_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:06.61 +15:11:07.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 203135_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203135_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:47.59 +13:22:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 5.392 3343596962942083328 090.19836078039 +13.37261480968 13.2596 12.4468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203137_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203137_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:44.02 +13:56:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203142_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203142_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203155_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203155_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:56.81 +13:25:53.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 203157_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203157_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:24.62 +13:27:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203163_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203163_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:32.61 +13:10:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.347 3346395872869652736 087.63533661239 +13.17355481623 13.5551 13.0582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203167_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203167_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:49.71 +13:49:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.239 3346830106945060480 087.95701030772 +13.82257681677 13.3339 12.7810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203170_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203170_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:33.36 +16:48:06.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203175_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203175_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:38.02 +13:10:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203180_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203180_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:14.35 +15:48:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203181_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203181_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:14.07 +13:48:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.631 3344428537329458816 092.55861845414 +13.80443576768 13.2925 12.6743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203194_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203194_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:10.39 +16:00:21.9 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 203213_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203213_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203217_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203217_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:09:00.32 +14:09:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 5.750 3345203143271695872 092.25140588413 +14.15845999959 13.5138 13.0777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203224_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203224_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203250_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203250_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:13.85 +13:11:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.792 3343359124833102464 088.55768877991 +13.19191907203 13.3453 12.6443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203268_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203268_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:25.19 +14:31:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203271_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203271_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:07:12.23 +14:04:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.515 3345117342706635648 091.80116743588 +14.06870674382 13.1408 12.1102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203273_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203273_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:12.67 +17:39:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.687 3350397167482260224 089.30285110720 +17.65236570234 13.3926 12.8955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203283_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203283_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:31.47 +15:36:11.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 203284_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203284_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:45.66 +09:59:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.493 3341742258624718592 089.69055207978 +09.98569802759 13.9047 13.3348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203300_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203300_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:24.53 +16:18:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.941 3357371850774022400 098.10201780105 +16.31130638763 13.0454 12.0051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203312_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203312_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:20:52.76 +16:28:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.605 3369216507285239296 095.21999695578 +16.47278443316 13.4907 12.9752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203316_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203316_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:31.55 +10:48:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.197 3341999883644048128 089.88111600940 +10.81266161092 13.1970 12.2588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203319_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203319_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203324_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203324_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:46.63 +16:49:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.210 3369393567314931712 096.94451270717 +16.82693324043 13.3832 12.8503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203330_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203330_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203335_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203335_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:52.59 +10:38:03.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)
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Considering the candidate 203336_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203336_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203340_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203340_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:59.91 +17:51:48.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203357_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203357_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203364_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203364_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203367_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203367_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:17.53 +12:14:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203375_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203375_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203378_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203378_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:11.99 +11:17:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 5.309 3337068406493385728 087.54956317409 +11.28563255882 13.5655 12.9609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203383_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203383_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203399_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203399_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203407_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203407_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:07.36 +12:35:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.378 3343267723631107456 089.03078684812 +12.59695608819 13.6855 13.2261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203410_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203410_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:56.80 +17:52:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.480 3350407544123197056 089.48629840031 +17.87882133075 13.4224 12.4898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203413_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203413_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:51.17 +17:55:14.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 203418_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203418_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:05.43 +17:21:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.654 3370453389145548160 095.27237363168 +17.35522975346 13.6181 13.1831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203420_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203420_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:54.88 +17:17:28.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 203424_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203424_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:30:25.29 +17:20:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.256 3369526603925834240 097.60511374302 +17.33440007229 13.4532 12.6703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203426_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203426_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:34.14 +11:02:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.062 3341915981461934592 090.39181586672 +11.04542746453 13.5229 12.6909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203431_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203431_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:20.07 +12:15:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.772 3343378263207910656 089.83334310327 +12.25587798965 13.4157 12.6307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203436_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203436_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203440_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203440_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:29.03 +13:52:04.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 203441_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203441_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203442_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203442_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203453_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203453_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203460_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203460_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203465_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203465_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:03.86 +14:04:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.416 3346887560726999424 089.51701825793 +14.07174834440 14.4755 13.6871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203472_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203472_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203480_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203480_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203486_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203486_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:05.48 +17:24:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.857 3370233937794496256 093.52297724165 +17.40113196020 13.6763 13.1406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203492_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203492_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:38.69 +13:05:59.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 203502_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203502_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203508_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203508_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:21.28 +17:00:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.727 3349743782697604864 089.83823275346 +17.00404764242 13.4454 12.9351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203512_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203512_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:44.05 +15:24:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203513_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203513_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203518_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203518_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203526_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203526_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:08.39 +14:35:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 5.415 3345299522337567232 092.03476892034 +14.58575701858 13.7165 13.1197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203531_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203531_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:24.80 +15:45:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 5.129 3348799920684849408 088.85319716402 +15.74958133421 13.4864 13.0783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203533_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203533_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203537_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203537_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203545_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203545_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203546_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203546_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:45.20 +14:33:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.692 3356132460651403008 099.18838350362 +14.55508651825 13.4724 13.1675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203548_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203548_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:16.84 +14:02:10.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 203564_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203564_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203567_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203567_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:02.81 +17:42:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 5.686 3371007890901909120 098.76159481610 +17.69847993389 13.6235 13.1420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203576_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203576_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:24.06 +17:40:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203580_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203580_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203582_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203582_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:16.93 +17:33:31.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)
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Considering the candidate 203593_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203593_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203594_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203594_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:12.82 +12:50:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 5.369 3332069923556110976 094.30346753071 +12.84378724923 13.6724 13.1760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203598_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203598_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:48.19 +15:23:34.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 203602_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203602_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:25.42 +11:56:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.549 3343155955700023168 087.60605152246 +11.93904880634 13.6624 13.1135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203614_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203614_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:44.97 +13:06:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 5.427 3332283297530696832 096.68762104408 +13.10270616573 13.2714 12.4362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203615_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203615_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:43.33 +10:26:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.053 3336019438039885952 088.67973659359 +10.44011868399 13.7016 12.8863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203628_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203628_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:35:10.12 +12:37:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.543 3355225672796911104 098.79222552796 +12.62498914517 13.2827 12.7618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203634_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203634_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:14.59 +14:31:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.103 3356646104381024640 096.56086069527 +14.52705744444 13.9520 13.3389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203644_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203644_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:44.40 +14:04:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.513 3355849194670986112 099.43449093866 +14.07185285923 13.6757 13.2306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203645_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203645_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203653_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203653_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:28.53 +14:16:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 4.505 3344804089271135360 093.86789478730 +14.27957439078 14.1119 13.5959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203659_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203659_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:42.92 +14:21:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.921 3347060321491428736 088.17848411495 +14.34987015175 13.3409 12.5665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203663_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203663_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203665_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203665_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203668_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203668_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:29.21 +14:24:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.522 3346876939268245376 088.62131814771 +14.41462458339 13.7117 13.2898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203670_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203670_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:00.55 +14:22:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.462 3346917488059002624 089.75326536911 +14.36716804620 13.7002 13.1066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203672_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203672_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203677_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203677_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203683_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203683_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:16.45 +15:16:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 5.832 3347227206739949568 088.81828406502 +15.26909363616 13.6108 13.1519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203689_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203689_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203690_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203690_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:57.22 +12:23:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.391 3343070674829431296 089.23852167394 +12.38453820299 13.8070 13.3884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203698_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203698_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:24.13 +14:13:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.470 3344791788484470656 093.35052498858 +14.22873089835 14.0035 13.0579 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 203702_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203702_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203703_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203703_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:05.01 +17:21:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.659 3369750255758706304 096.76992678425 +17.35715835703 13.9769 13.6274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203718_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203718_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:59.08 +14:56:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.757 3356723963548046720 096.49593223870 +14.94388926724 13.4257 12.5028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203721_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203721_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:59.48 +15:38:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203722_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203722_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203725_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203725_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:52.94 +13:28:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.285 3346419993405922688 087.47086539119 +13.46842504712 13.7153 12.9254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203732_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203732_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:11.94 +12:16:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.406 3343378911745513600 089.79975530818 +12.27227598907 13.7335 13.3991 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 203733_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203733_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:20:38.86 +15:42:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.785 3369030208782864768 095.16164666202 +15.69908082032 13.4126 12.7424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203741_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203741_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:36.98 +14:40:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.088 3347872345187595520 087.40284980173 +14.66771469263 13.6313 13.0201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203745_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203745_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:41:53.66 +16:17:27.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 203751_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203751_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:30.86 +16:22:26.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 203757_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203757_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:01.99 +14:27:32.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 203760_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203760_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203764_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203764_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:45.33 +13:40:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203768_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203768_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:51.55 +12:24:02.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 203769_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203769_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:21.45 +11:26:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.996 3342293285749216768 091.58921954162 +11.43270391579 13.6667 13.1442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203772_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203772_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203773_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203773_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:23.61 +10:44:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 4.516 3341890280378126464 090.34846684556 +10.73772091921 13.7368 13.4181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203774_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203774_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:40:04.16 +16:12:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203776_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203776_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203778_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203778_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203779_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203779_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:26.65 +17:40:48.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 203782_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203782_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203789_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203789_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:39.23 +11:43:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.671 3331139015162664960 097.41324757429 +11.72494123221 13.4556 12.9486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203795_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203795_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:26.79 +11:52:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.114 3342554041803119744 091.11160799284 +11.87555177583 13.7394 13.1750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203800_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203800_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:17.21 +12:35:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.927 3346220844361968640 087.82172887290 +12.58604808586 13.5963 13.2071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203803_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203803_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:02.62 +11:51:51.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)
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Considering the candidate 203812_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203812_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:00.83 +18:02:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 5.889 3350331162424218368 090.25327253217 +18.03384602834 13.8045 13.3758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203816_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203816_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:08:19.33 +11:24:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.340 3342280813164107904 092.08007562927 +11.41108871148 13.8708 13.5181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203818_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203818_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203820_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203820_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:56.94 +15:40:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.401 3348785833192099456 088.98692511491 +15.67283834977 13.6113 13.0436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203826_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203826_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:33.43 +14:52:28.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)
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Considering the candidate 203828_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203828_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:55.43 +13:07:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 5.508 3343541781202479872 090.98132666320 +13.11992942365 13.6785 12.8448 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203847_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203847_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:48:53.63 +10:23:23.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 203851_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203851_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:46.92 +13:55:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.471 3345330583541793152 090.69587578830 +13.92552475657 13.7644 13.2141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203858_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203858_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:24:19.70 +15:59:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203866_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203866_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203877_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203877_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:21.86 +14:28:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.481 3346936592073193600 089.34178083077 +14.47459341375 13.4048 12.6377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203878_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203878_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203886_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203886_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203889_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203889_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203891_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203891_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:24:23.57 +13:02:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 5.523 3332267285892796800 096.09763539836 +13.03365419127 13.6667 13.1735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203892_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203892_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:33:19.47 +18:04:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.682 3371082382814210944 098.33138212551 +18.06972269078 13.7119 13.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203894_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203894_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:24:26.54 +15:51:15.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 203896_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203896_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203900_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203900_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:19:42.81 +11:01:40.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 203901_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203901_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203907_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203907_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:09.87 +15:54:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.586 3368944275077008128 096.29075182482 +15.90046270267 13.7162 13.1368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203908_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203908_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203917_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203917_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:57.03 +12:14:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.017 3343051089778622464 089.23769903909 +12.24546925573 13.8166 13.2858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203924_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203924_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:18.08 +15:56:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203926_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203926_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203932_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203932_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203940_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203940_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203942_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203942_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203951_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203951_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:36.60 +12:15:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.996 3331968115652147840 094.15247833434 +12.26200137289 13.3253 12.4223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203969_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203969_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203971_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203971_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203975_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203975_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:42.52 +18:05:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.306 3371314100594722048 097.17742183438 +18.09499536501 13.7279 13.1675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203980_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203980_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203981_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203981_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 203984_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203984_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:27.88 +16:54:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 4.371 3349783330756377344 088.86595343350 +16.91499756788 13.9028 13.4313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203985_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203985_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:54.38 +17:17:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.248 3369658167363724928 096.47609072572 +17.29742569394 13.5208 13.1639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203990_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 203990_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203996_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 203996_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:56.40 +16:11:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.195 3357146347810392064 099.23479689737 +16.18373693002 13.4610 12.9240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204000_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204000_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204002_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204002_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:33.72 +17:04:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.268 3349794291512878592 088.89081554739 +17.06736612998 13.7714 13.4247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204009_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204009_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:09.27 +17:17:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 5.727 3369513792039011328 098.03791458587 +17.28594988516 13.7527 13.1458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204011_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204011_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:05:26.51 +12:45:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 5.550 3342766591144312704 091.36026810849 +12.76094163387 13.7451 13.2045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204012_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204012_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:02.33 +15:01:14.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 204015_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204015_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204017_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204017_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204018_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204018_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204019_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204019_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:15.87 +15:24:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.709 3348602283468997504 091.06602424260 +15.41561331360 14.0165 13.4935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204023_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204023_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:56.65 +18:06:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 5.828 3350297386801211776 090.98632411144 +18.10023689286 13.6378 13.0475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204029_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204029_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204037_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204037_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:16.98 +17:47:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204039_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204039_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:30.26 +11:35:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 5.632 3337140974260785408 087.37602155482 +11.58538122826 13.6127 13.0112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204057_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204057_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:09.86 +16:18:45.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 204068_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204068_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:43.10 +17:27:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204070_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204070_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:02.77 +09:55:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.780 3329872579628975872 092.51147589401 +09.92664603025 13.6061 13.0776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204072_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204072_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:26.77 +12:46:35.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 204075_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204075_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:26.77 +17:05:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204077_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204077_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:52.37 +13:36:29.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
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Considering the candidate 204078_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204078_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204081_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204081_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:23.66 +14:28:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.326 3346936695152404480 089.34925582038 +14.48032327888 13.6926 13.1660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204083_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204083_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204085_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204085_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204090_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204090_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204093_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204093_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:57.20 +14:11:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.226 3344605902299249664 094.23820934964 +14.18649888770 13.4499 12.5087 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 204095_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204095_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:25.45 +13:59:23.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)
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Considering the candidate 204096_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204096_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:09.11 +11:49:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.783 3343114552215565568 088.28773570556 +11.82960280169 14.2790 13.4888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204102_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204102_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:35.55 +12:10:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 5.792 3343222368776542848 088.64813333114 +12.16544661888 13.7980 13.1349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204107_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204107_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204109_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204109_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:58.47 +13:20:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 5.369 3332480488069592064 094.49408703400 +13.33407798648 14.1866 13.4502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204113_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204113_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204119_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204119_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:12.23 +11:43:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204123_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204123_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204137_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204137_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:32.60 +17:42:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 5.281 3350213961356368256 089.63560695884 +17.70863236355 13.4533 12.4621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204140_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204140_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:34.22 +10:21:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.075 3329995419991336960 093.39253521984 +10.35520212878 14.0004 13.5740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204141_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204141_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204144_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204144_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:36.99 +14:18:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.535 3344622257534706560 094.15406798562 +14.30018582123 13.7200 12.8691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204145_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204145_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204152_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204152_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204160_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204160_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:32:43.15 +12:49:06.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204166_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204166_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:00.64 +17:02:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204170_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204170_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:14.86 +13:49:33.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204172_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204172_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204177_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204177_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204179_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204179_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:56.22 +14:18:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204180_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204180_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204181_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204181_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:34:46.10 +16:09:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204189_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204189_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:32.01 +13:11:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.846 3344141972817798528 093.13354346186 +13.19463435012 13.7028 13.1604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204192_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204192_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:52.44 +15:34:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.615 3345046428504871552 094.21898502438 +15.57628979007 14.2092 13.5514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204202_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204202_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:01.93 +17:01:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 5.740 3369596839526811008 096.50838554566 +17.02746764185 13.6130 13.1678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204210_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204210_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204212_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204212_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:25.59 +10:52:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.036 3341872271578063744 090.85663498183 +10.86646214116 14.0782 13.6303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204215_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204215_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204218_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204218_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:28.85 +12:44:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 5.302 3343306416994666368 088.37033911616 +12.74297721180 13.8409 13.0228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204220_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204220_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:22:45.92 +17:35:33.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204224_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204224_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204229_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204229_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204231_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204231_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:31.96 +17:39:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 5.487 3350025910509431808 089.13264464062 +17.65453140846 14.0568 13.5584 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204238_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204238_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204240_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204240_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204248_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204248_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204249_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204249_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:53.16 +10:54:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.814 3341863956521497088 091.22144963199 +10.89935791620 13.7683 13.3700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204253_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204253_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204259_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204259_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:52:14.69 +13:24:30.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204266_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204266_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:38.99 +16:53:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 4.792 3349771472349737984 088.91254885901 +16.89197738060 13.7111 12.8717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204267_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204267_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:27.27 +14:57:43.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204269_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204269_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:26.85 +11:42:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.140 3342951888915342464 089.36174956629 +11.70143857283 13.7513 13.2688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204270_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204270_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:15.95 +13:45:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.456 3346812171164410880 088.31641262274 +13.75865174670 13.7832 13.3570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204278_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204278_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204281_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204281_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204282_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204282_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:07:29.80 +09:59:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204297_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204297_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204302_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204302_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:51.06 +15:09:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.084 3368779176534953856 095.46244464931 +15.16526550421 13.6108 12.7308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204303_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204303_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204306_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204306_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:36.11 +12:04:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 5.615 3343184302483922048 087.89999352359 +12.07736909999 13.8355 13.2224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204307_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204307_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204311_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204311_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204313_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204313_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204319_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204319_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204335_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204335_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:05.64 +14:12:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 5.893 3343914172047013248 090.02347495254 +14.21289096570 13.9893 13.6189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204344_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204344_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:31.86 +11:59:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.564 3342995152124616320 089.38246282233 +11.99445805621 13.9131 13.3876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204364_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204364_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204369_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204369_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:16.33 +16:56:31.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 204378_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204378_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:38.61 +14:21:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 5.480 3345361953982546560 090.66096814153 +14.36025821167 13.9148 13.2457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204391_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204391_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204393_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204393_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:54.45 +17:32:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 5.087 3370240431785028864 093.47626053637 +17.54568642566 13.1651 11.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204396_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204396_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:06.53 +10:34:44.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204397_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204397_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:02.37 +15:42:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 5.349 3348763980398770176 089.50979634160 +15.70048828735 14.1207 13.5462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204410_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204410_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204430_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204430_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204431_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204431_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204432_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204432_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204434_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204434_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204436_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204436_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:59.69 +15:33:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 5.480 3348643102838021376 090.24878041303 +15.56250708841 13.8900 13.5023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204441_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204441_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:39:16.78 +15:47:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.839 3358560663362094976 099.81982881469 +15.78524179564 13.7950 13.0249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204461_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204461_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204462_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204462_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204473_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204473_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:38:59.12 +18:06:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.636 3359120104325394048 099.74592801634 +18.11114931213 13.6597 12.8101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204474_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204474_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:38.70 +14:50:42.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 204478_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204478_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204482_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204482_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204483_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204483_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:28:32.29 +13:51:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204484_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204484_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:33:13.72 +15:44:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.602 3357199845925061120 098.30691407873 +15.74211272344 13.8014 13.2330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204493_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204493_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:02:49.37 +12:58:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 5.239 3343527109594291712 090.70578778865 +12.98013013461 13.9841 13.4226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204497_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204497_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:56.27 +16:55:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 5.718 3349774569023465216 089.23484774192 +16.92512264185 13.9334 13.3776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204500_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204500_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204520_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204520_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204525_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204525_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:32.55 +17:39:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.762 3369740153995181568 097.38566101082 +17.66292771964 13.7939 13.3567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204529_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204529_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204538_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204538_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:27:30.46 +15:11:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 5.198 3356816528683406208 096.87668311964 +15.18893501446 13.7874 12.9522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204540_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204540_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204546_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204546_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:31.78 +15:12:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 5.710 3347212122815249408 089.13228903948 +15.20186300758 14.1492 13.6009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204548_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204548_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:34.45 +13:53:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 5.122 3346788192363207680 089.14459166093 +13.89186850965 13.8143 13.5799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204552_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204552_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:02.69 +17:05:12.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)
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Considering the candidate 204554_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204554_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204557_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204557_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204558_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204558_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204559_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204559_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204567_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204567_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:06.39 +11:12:58.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 204573_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204573_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:29.73 +16:02:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 5.815 3346058047922104320 092.62334485148 +16.03960598569 14.3679 13.6974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204574_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204574_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204577_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204577_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204582_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204582_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204584_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204584_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204586_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204586_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:06.84 +18:01:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.837 3370504344640098304 095.77809727727 +18.01572765821 13.7654 13.0399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204590_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204590_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204593_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204593_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204595_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204595_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204600_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204600_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:48.91 +15:29:12.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 204603_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204603_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204605_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204605_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204611_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204611_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204627_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204627_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:22.15 +14:21:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 5.684 3345277532104880640 091.59289609414 +14.35936711403 14.1099 13.5229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204628_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204628_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204635_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204635_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:28.58 +13:53:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 5.068 3344582537677281664 093.86862024652 +13.89844366479 14.1967 13.6744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204644_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204644_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204647_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204647_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:19.87 +11:39:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 5.289 3342911967197644800 088.83263984573 +11.65573293740 14.0060 13.2508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204652_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204652_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204653_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204653_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204654_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204654_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:58.81 +14:03:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 5.402 3344553538058231424 094.49466129482 +14.06407318313 13.5049 12.3317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204659_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204659_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204665_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204665_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:14.05 +13:29:51.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 204676_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204676_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:50:48.56 +15:39:15.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)
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Considering the candidate 204682_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204682_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204688_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204688_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204691_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204691_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:20.19 +16:40:10.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
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Considering the candidate 204699_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204699_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204700_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204700_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204702_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204702_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:21:05.17 +11:35:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204703_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204703_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:13.90 +13:00:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 4.738 3344055184412449792 092.80765864825 +13.00898576703 14.6305 14.0798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204711_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204711_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 204714_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204714_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:52.36 +09:56:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204718_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204718_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204720_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204720_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:27.15 +17:23:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 5.817 3370421297151151360 095.86275288095 +17.38456259755 14.0944 13.4990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204723_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204723_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:14.94 +16:01:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 5.094 3348686739705512960 090.81235708017 +16.02483865871 14.1625 13.6222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204726_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204726_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204730_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204730_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:37:24.43 +16:26:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 5.853 3358655049562574080 099.35116996417 +16.44301524045 14.1747 13.8275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204741_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204741_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:14.91 +13:30:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204746_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204746_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204748_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204748_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204760_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204760_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:06:59.44 +10:59:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 4.500 3330233872278524544 091.74778466200 +10.98317196067 14.0953 13.1854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204771_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204771_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204772_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204772_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204775_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204775_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:36:09.04 +13:10:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.876 3355402419291181824 099.03689489288 +13.18117331440 14.1767 13.5658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204777_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204777_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204781_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204781_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204782_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204782_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:25:40.33 +17:47:38.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)
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Considering the candidate 204793_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204793_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204803_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204803_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204811_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204811_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204814_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204814_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204819_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204819_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:54:49.59 +11:21:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 5.732 3342851184820631040 088.70666331209 +11.35974146105 14.3702 13.9379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204820_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204820_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204838_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204838_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:49.21 +15:12:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 5.572 3347223117931582080 088.95540874545 +15.21332663890 14.1250 13.7022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204859_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204859_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204870_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204870_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204874_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204874_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:16:11.10 +14:06:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 5.206 3344610467845907840 094.04660218385 +14.10401161333 13.8377 12.8891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204876_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204876_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:49.28 +16:02:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204877_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204877_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:58:27.25 +14:27:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 5.491 3346933770276361088 089.61426617952 +14.45539575712 14.0898 13.5683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204883_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204883_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204886_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204886_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:15.25 +16:07:30.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)
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Considering the candidate 204897_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204897_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:20.27 +11:45:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 5.475 3342952374250843392 089.33442279325 +11.75175724512 14.1175 13.9189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204899_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204899_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204901_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204901_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204905_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204905_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204923_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204923_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204932_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204932_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204940_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204940_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:09.32 +10:26:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 5.473 3329953054433697536 092.53819326247 +10.43483841411 14.2273 13.5625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204944_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204944_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204946_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204946_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:37.74 +15:33:35.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)
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Considering the candidate 204973_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204973_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204979_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 204979_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 204981_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 204981_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:29:57.12 +16:27:17.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)
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Considering the candidate 205009_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205009_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:52.06 +13:50:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 4.938 3346830313103564032 087.96754289848 +13.83568727043 14.1301 13.5948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205021_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205021_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205039_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205039_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205070_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205070_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205081_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205081_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205087_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205087_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205093_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205093_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:00:54.58 +15:22:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 4.119 3348543219079128064 090.22765662467 +15.36974052227 14.0443 13.0701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205099_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205099_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205101_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205101_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:59:27.04 +14:40:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205103_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205103_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205124_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205124_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205146_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205146_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:51:10.31 +12:58:46.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)
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Considering the candidate 205151_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205151_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:49:23.14 +14:09:25.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)
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Considering the candidate 205173_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205173_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:23:13.05 +10:04:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.380 3330464739659340672 095.80452654235 +10.07021704013 14.3971 13.7810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205178_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205178_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205186_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205186_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:45.26 +12:01:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 5.364 3331868919086572544 093.93813891712 +12.01643580254 14.0305 13.0225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205199_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205199_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:54.51 +15:42:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 5.238 3348792533341075968 088.97726553043 +15.69880130651 14.1904 13.5577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205211_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205211_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205213_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205213_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205214_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205214_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205217_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205217_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:38.03 +16:36:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 5.509 3349293086008130176 090.40929792319 +16.60067049956 14.4445 13.9155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205222_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205222_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:26:38.08 +13:19:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205224_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205224_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:58.55 +17:49:09.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)
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Considering the candidate 205227_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205227_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205230_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205230_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205231_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205231_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205234_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205234_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205248_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205248_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205254_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205254_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:55:56.02 +14:18:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 4.701 3346951985236173952 088.98435411083 +14.31092298474 14.3934 13.6833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205256_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205256_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205258_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205258_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:53:47.68 +15:27:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 5.648 3347290050701469696 088.44840971863 +15.46367306759 14.3471 13.8320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205267_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205267_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:41.06 +12:23:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 5.525 3331976258910007168 094.42122738592 +12.39816632008 14.4919 13.9333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205284_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205284_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205296_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205296_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:19.09 +14:18:37.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
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Considering the candidate 205302_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205302_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:57.69 +13:40:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205311_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205311_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205316_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205316_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205320_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205320_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205323_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205323_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205336_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205336_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:57.42 +18:13:01.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)
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Considering the candidate 205337_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205337_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205343_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205343_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:57:28.76 +17:32:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 5.284 3350207845322997376 089.36997933457 +17.54545542136 14.3254 13.7617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205353_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205353_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:03:34.22 +15:37:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205361_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205361_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:01:53.87 +15:48:14.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)
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Considering the candidate 205368_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205368_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205387_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205387_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205391_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205391_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205394_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205394_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205403_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205403_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205412_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205412_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:15.84 +13:00:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205418_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205418_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205420_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205420_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:04:16.28 +12:46:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205430_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205430_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205438_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205438_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205439_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205439_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205448_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205448_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205454_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205454_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:17:55.27 +14:48:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205462_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205462_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205465_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205465_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205475_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205475_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:15:01.98 +16:29:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205483_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205483_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205484_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205484_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205486_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205486_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:10:38.37 +15:03:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 4.833 3345692632104572288 092.66005031604 +15.06272381904 14.8505 14.1446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205493_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205493_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205501_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205501_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205503_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205503_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 05:56:04.37 +13:53:44.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 205505_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205505_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205506_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205506_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205508_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205508_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205510_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205510_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205511_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205511_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205520_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205520_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205534_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205534_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:12:25.14 +14:00:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 5.691 3344411524961061760 093.10384746899 +13.99971155679 14.5583 13.9449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205543_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205543_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205574_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 205574_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
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Considering the candidate 205579_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205579_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:11:27.76 +11:53:59.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)
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Considering the candidate 205589_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205589_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:55.11 +16:54:21.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)
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Considering the candidate 205673_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205673_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:13:48.61 +12:46:49.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)
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Considering the candidate 205759_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
The candidate 205759_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058 did not pass the final checks
**** FOUND 06:14:22.94 +12:07:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124797_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
Preparing report for the candidate 124797_fd_Ori-02-Q2b1x1_2026-03-28_21-56-20_20.00sec_-15.00C_LIGHT_0058
make_report_in_HTML.sh Phase 2 (HTML assembly): 76s
make_report_in_HTML.sh TOTAL: 765s
Prepared the HTML report for the field Ori-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:35:44.72 +11:17:02.2
05:58:23.72 +11:50:43.1
06:04:11.35 +12:35:21.9
06:14:35.48 +11:15:30.7
06:01:33.03 +12:58:52.5
06:13:19.53 +14:42:59.0
06:11:39.40 +15:01:29.1
06:00:51.32 +16:19:51.9
06:08:32.34 +12:55:13.0
06:15:54.44 +12:55:37.6
05:58:30.36 +17:12:37.4
05:58:29.54 +15:03:34.6
06:28:29.58 +15:24:33.8
06:11:23.33 +15:36:18.7
06:11:51.37 +15:43:45.7
05:56:00.70 +11:46:10.3
06:08:22.48 +11:49:59.2
05:50:15.94 +13:54:06.7
06:11:31.89 +13:26:07.7
06:32:37.70 +17:57:41.0
05:50:13.32 +13:10:47.3
05:52:57.06 +13:18:07.9
06:01:37.27 +15:19:51.9
06:01:45.31 +11:15:08.8
06:02:38.41 +14:07:58.5
06:31:46.63 +18:03:22.1
06:06:13.09 +16:19:25.9
05:59:02.80 +14:46:12.3
06:02:21.36 +16:12:34.2
06:08:27.07 +16:23:02.2
06:30:27.64 +13:42:19.9
05:55:28.40 +12:46:35.7
05:55:21.77 +15:39:09.2
06:04:18.72 +12:32:52.4
06:09:52.59 +14:42:45.0
05:52:23.63 +14:54:07.5
06:26:01.11 +16:56:24.1
06:10:22.29 +16:14:32.2
06:34:28.25 +17:43:05.2
06:01:12.93 +14:02:43.4
06:00:38.09 +15:37:19.4
06:31:42.38 +16:47:43.8
06:00:38.27 +15:56:45.7
06:11:44.51 +17:21:10.0
06:27:07.91 +16:55:02.4
05:57:44.30 +13:34:32.9
06:21:43.42 +12:44:20.6
05:51:44.66 +14:17:01.2
06:07:08.68 +12:32:31.1
06:08:08.26 +14:27:05.4
06:15:50.94 +17:58:52.8
05:57:00.12 +13:28:56.6
06:15:32.34 +13:47:36.2
06:13:27.53 +14:13:51.9
06:10:32.45 +16:29:31.2
05:54:18.55 +15:25:19.1
05:54:12.38 +15:02:21.1
05:57:35.31 +17:58:56.7
06:02:12.38 +12:06:06.2
05:55:30.15 +15:07:43.0
06:38:24.91 +16:31:42.9
06:07:05.39 +10:57:47.3
06:12:20.08 +10:02:02.9
06:01:14.33 +14:32:07.9
05:49:53.50 +12:29:45.4
06:02:09.67 +12:11:04.5
06:17:55.26 +14:42:53.9
06:17:02.23 +15:48:27.1
06:20:26.34 +17:59:04.0
06:15:57.83 +15:45:45.1
05:51:24.63 +13:40:34.6
06:31:29.54 +15:00:32.2
05:54:03.01 +13:05:40.2
05:52:22.26 +14:25:29.3
05:54:02.77 +14:48:32.4
06:37:48.45 +13:57:17.5
05:55:31.00 +15:11:03.4
06:03:54.47 +12:44:04.2
06:03:24.37 +14:38:53.9
06:00:15.12 +10:00:43.1
06:38:17.59 +13:56:19.0
06:28:19.35 +16:19:07.2
06:15:53.67 +14:10:16.5
06:25:36.63 +13:37:50.3
05:57:33.47 +10:55:27.7
06:00:12.83 +10:48:38.6
06:32:24.25 +14:54:07.7
06:09:12.73 +15:40:26.2
06:41:18.37 +18:02:06.5
06:11:23.67 +14:49:43.8
05:50:05.21 +10:34:52.9
05:52:18.21 +15:51:58.5
06:13:49.71 +12:47:05.9
06:16:19.10 +12:58:42.3
06:12:48.01 +15:57:44.1
06:32:06.16 +18:09:36.7
05:59:04.15 +15:40:37.4
06:41:47.79 +16:51:34.7
05:58:02.29 +16:49:20.9
06:36:42.85 +11:12:37.7
05:57:29.14 +16:25:49.5
05:57:55.44 +13:34:11.1
06:38:09.24 +15:02:40.6
06:20:24.74 +14:14:42.3
05:52:33.54 +15:43:51.8
06:06:40.77 +15:11:24.5
06:13:23.70 +17:13:26.2
05:51:05.92 +15:39:54.3
06:00:36.43 +11:03:23.1
06:21:53.66 +13:08:31.1
06:26:36.79 +17:47:21.8
06:40:09.43 +14:33:37.8
05:55:57.23 +16:32:15.4
05:56:51.70 +12:21:05.0
06:17:44.87 +14:40:48.6
06:21:40.48 +17:48:04.2
05:48:32.31 +11:28:52.5
06:13:17.34 +11:55:02.2
06:11:10.67 +17:30:32.5
06:26:25.39 +17:42:20.4
05:56:53.22 +14:50:24.1
06:03:45.62 +14:20:46.8
06:16:27.35 +16:42:37.0
06:10:11.93 +17:42:34.7
06:05:20.88 +15:10:13.7
06:19:42.37 +15:59:26.5
05:57:13.85 +17:30:31.4
05:57:47.55 +14:19:56.9
06:35:06.81 +12:37:59.2
06:13:39.25 +12:47:36.1
06:17:11.07 +15:50:13.9
06:06:57.44 +18:07:52.5
05:58:23.29 +14:59:59.7
05:56:44.03 +17:00:10.6
06:22:11.59 +16:05:21.9
06:10:30.86 +14:52:41.5
06:09:52.24 +11:19:55.9
06:36:13.58 +13:05:53.3
06:08:14.29 +13:57:07.0
06:17:52.57 +15:42:08.5
06:23:30.72 +15:36:13.9
06:15:00.70 +14:58:53.8
06:00:20.50 +15:32:27.3
06:18:18.07 +14:22:18.5
06:01:23.34 +13:54:28.3
06:14:42.27 +15:10:59.3
06:25:09.40 +15:58:53.2
06:12:57.12 +17:26:20.8
05:59:57.47 +13:03:23.9
06:14:37.19 +16:02:30.0
06:26:56.70 +16:47:33.6
06:07:01.07 +10:58:45.7
06:22:17.55 +14:40:26.2
05:53:52.19 +10:13:57.5
05:49:29.16 +13:54:40.7
06:12:28.12 +15:20:04.0
06:11:37.12 +15:28:25.8
05:52:38.40 +15:49:35.6
06:12:18.14 +15:12:21.6
05:58:27.75 +14:56:55.0
06:34:47.10 +15:31:02.4
06:00:02.61 +11:09:52.3
06:00:51.40 +10:59:28.2
06:19:47.12 +16:38:52.2
05:52:46.77 +15:24:02.9
06:11:09.03 +17:31:03.4
06:17:01.32 +18:06:38.1
06:12:21.10 +15:28:31.8
06:27:16.30 +15:59:50.2
06:16:19.71 +14:31:17.4
06:21:47.10 +17:02:50.5
05:50:50.22 +14:25:30.8
06:13:44.01 +14:52:17.4
05:57:13.85 +17:08:13.1
06:15:27.96 +14:23:53.8
05:52:19.39 +15:41:14.0
06:19:12.08 +12:45:05.6
06:06:58.48 +14:36:07.6
06:18:12.86 +17:18:43.0
06:27:44.20 +17:39:44.9
06:14:33.77 +14:45:32.8
06:03:52.31 +14:59:06.2
06:27:05.36 +15:18:40.6
06:25:36.83 +14:06:33.7
05:59:07.20 +15:23:10.3
06:12:31.19 +15:20:14.8
06:12:58.78 +16:22:06.4
06:26:01.08 +16:39:51.4
06:17:50.72 +16:23:57.8
05:58:48.36 +13:38:12.1
06:14:14.15 +13:14:59.7
05:48:08.74 +15:56:46.3
05:54:30.48 +12:57:31.2
05:57:54.95 +15:49:12.1
06:18:54.39 +11:33:58.2
06:03:20.61 +10:39:27.7
06:00:57.41 +16:27:52.0
05:56:21.71 +17:58:16.1
05:56:34.56 +10:29:34.4
06:33:00.95 +16:03:44.3
05:51:00.51 +13:29:08.8
06:02:23.83 +16:35:57.0
06:11:05.92 +16:19:10.0
05:55:47.19 +14:48:03.3
06:13:31.18 +17:23:07.5
05:57:00.08 +17:55:39.2
06:09:55.61 +14:26:05.8
06:14:08.40 +17:22:59.2
05:55:13.00 +12:41:16.7
06:20:58.44 +14:41:23.0
06:20:57.41 +16:50:14.0
06:27:51.97 +16:41:06.2
06:19:32.57 +13:26:12.2
05:53:13.24 +14:40:26.3
06:14:22.25 +10:07:40.1
05:49:14.22 +14:41:49.9
05:50:03.76 +10:24:30.6
06:12:26.70 +15:00:24.6
06:01:37.68 +14:43:11.4
06:14:35.97 +13:49:52.3
06:06:48.48 +16:40:37.7
06:05:37.22 +17:10:44.5
06:18:28.69 +14:20:27.4
06:08:55.81 +17:07:39.8
05:55:56.50 +14:38:13.7
06:17:35.47 +14:21:38.3
05:49:16.39 +11:26:25.1
06:15:10.86 +14:43:50.2
06:18:34.84 +14:20:07.9
06:09:57.09 +16:59:12.5
05:58:48.37 +16:29:35.8
06:36:15.89 +17:59:27.2
06:10:46.63 +14:47:20.1
05:57:33.70 +15:38:37.6
06:00:21.97 +10:05:26.5
06:02:09.43 +13:56:17.9
06:00:57.68 +14:31:57.1
06:20:46.73 +15:42:08.3
06:06:05.15 +13:21:02.3
06:23:30.13 +11:14:21.5
05:58:26.36 +15:59:27.8
06:15:37.99 +17:53:12.9
06:17:24.85 +10:19:34.6
05:58:07.30 +16:38:48.8
05:48:53.13 +10:13:09.1
06:10:25.45 +13:28:04.0
05:49:28.19 +11:30:41.1
06:05:57.84 +11:37:35.4
06:19:04.36 +16:47:19.7
06:16:58.67 +18:09:12.6
06:11:38.99 +15:16:52.1
06:04:28.03 +16:29:14.2
06:21:31.34 +14:40:25.4
06:00:15.39 +12:08:18.0
05:57:29.86 +16:51:07.0
06:17:27.80 +11:05:42.3
06:06:00.97 +16:53:36.4
06:25:33.68 +17:35:13.7
05:56:04.67 +16:54:40.0
05:59:56.19 +11:30:34.1
06:17:11.51 +12:04:06.2
06:23:49.20 +16:28:13.7
05:50:25.64 +14:39:13.4
05:59:14.49 +14:14:26.2
06:11:59.01 +17:22:43.5
06:06:48.49 +16:49:38.2
06:24:49.25 +16:41:34.4
06:04:31.59 +15:26:09.2
06:14:21.65 +14:20:39.0
06:14:07.62 +18:00:35.7
06:01:42.11 +16:14:30.9
06:20:01.74 +13:52:51.3
06:04:26.30 +18:02:07.7
06:25:04.23 +16:36:40.2
06:01:19.48 +15:34:36.6
05:58:27.76 +15:59:40.1
06:10:54.56 +14:51:53.8
05:59:32.63 +13:11:26.7
06:18:42.41 +17:53:58.5
06:19:02.13 +16:47:08.0
05:56:16.27 +12:14:41.5
05:51:31.58 +15:47:51.0
06:20:39.35 +13:04:20.9
06:15:27.39 +14:45:49.8
05:57:29.25 +10:49:42.8
06:10:28.12 +13:50:01.6
05:50:15.64 +13:10:20.9
06:13:50.81 +14:44:31.5
06:07:09.40 +16:42:46.9
06:25:46.57 +17:09:24.5
05:59:11.19 +16:41:15.8
06:26:02.09 +15:47:59.3
05:58:52.27 +13:37:22.3
05:51:44.60 +15:34:43.5
05:51:19.82 +13:57:03.9
06:13:47.44 +15:24:03.1
06:16:28.87 +15:12:39.8
06:01:20.72 +17:26:15.5
05:55:50.23 +17:41:16.2
06:20:42.81 +17:46:45.8
06:19:59.21 +17:10:05.3
05:52:03.63 +15:17:57.9
05:52:24.06 +13:07:42.1
05:57:35.03 +15:59:00.1
05:57:42.27 +15:57:13.2
06:02:07.56 +15:11:23.2
06:13:10.18 +12:55:19.3
05:59:54.48 +16:54:38.7
06:19:36.57 +17:40:29.3
06:20:16.95 +13:20:08.4
05:55:56.82 +17:18:04.4
05:55:03.80 +15:54:25.8
05:58:30.34 +17:44:47.9
05:57:06.30 +17:40:03.3
06:27:31.25 +15:16:12.9
05:50:07.25 +15:27:57.1
05:56:47.22 +17:56:00.9
06:04:09.22 +15:25:54.2
05:57:37.01 +16:32:37.8
06:18:00.48 +17:37:01.4
05:48:37.32 +15:50:58.7
05:51:06.30 +15:03:04.4
05:56:09.13 +17:46:33.2
06:05:46.85 +10:58:59.2
06:02:07.79 +16:23:46.6
06:06:25.19 +16:38:04.6
05:55:23.29 +14:46:09.8
05:54:30.03 +14:48:43.8
05:51:14.90 +14:02:32.7
06:20:35.52 +13:38:05.2
05:56:33.13 +15:24:54.7
06:18:21.39 +17:01:39.7
05:59:25.67 +15:07:24.7
05:56:40.30 +16:06:18.8
06:01:21.00 +12:23:32.8
06:09:30.91 +13:08:59.7
05:59:57.80 +17:18:57.4
05:50:27.70 +15:04:18.3
05:53:11.70 +14:46:13.7
06:18:51.02 +14:40:00.2
05:56:00.89 +15:07:20.7
06:21:30.97 +15:43:18.3
06:10:55.00 +17:26:53.0
06:15:16.16 +15:59:57.2
05:49:48.99 +11:48:49.0
06:21:23.34 +13:14:45.8
########### Completed Ori-02-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 ####
06:35:44.72 +11:17:02.2
06:04:11.35 +12:35:21.9
06:14:35.48 +11:15:30.7
06:01:33.03 +12:58:52.5
06:13:19.53 +14:42:59.0
06:11:39.40 +15:01:29.1
06:00:51.32 +16:19:51.9
06:08:32.34 +12:55:13.0
06:15:54.44 +12:55:37.6
05:58:30.36 +17:12:37.4
05:58:29.54 +15:03:34.6
06:28:29.58 +15:24:33.8
06:11:23.33 +15:36:18.7
06:11:51.37 +15:43:45.7
05:56:00.70 +11:46:10.3
06:08:22.48 +11:49:59.2
05:50:15.94 +13:54:06.7
06:11:31.89 +13:26:07.7
06:32:37.70 +17:57:41.0
05:50:13.32 +13:10:47.3
05:52:57.06 +13:18:07.9
06:01:37.27 +15:19:51.9
06:01:45.31 +11:15:08.8
06:02:38.41 +14:07:58.5
06:31:46.63 +18:03:22.1
06:06:13.09 +16:19:25.9
05:59:02.80 +14:46:12.3
06:02:21.36 +16:12:34.2
06:08:27.07 +16:23:02.2
06:30:27.64 +13:42:19.9
05:55:28.40 +12:46:35.7
05:55:21.77 +15:39:09.2
06:04:18.72 +12:32:52.4
06:09:52.59 +14:42:45.0
05:52:23.63 +14:54:07.5
06:26:01.11 +16:56:24.1
06:10:22.29 +16:14:32.2
06:34:28.25 +17:43:05.2
06:01:12.93 +14:02:43.4
06:00:38.09 +15:37:19.4
06:31:42.38 +16:47:43.8
06:00:38.27 +15:56:45.7
06:11:44.51 +17:21:10.0
06:27:07.91 +16:55:02.4
05:57:44.30 +13:34:32.9
06:21:43.42 +12:44:20.6
05:51:44.66 +14:17:01.2
06:07:08.68 +12:32:31.1
06:08:08.26 +14:27:05.4
06:15:50.94 +17:58:52.8
05:57:00.12 +13:28:56.6
06:15:32.34 +13:47:36.2
06:13:27.53 +14:13:51.9
06:10:32.45 +16:29:31.2
05:54:18.55 +15:25:19.1
05:54:12.38 +15:02:21.1
05:57:35.31 +17:58:56.7
06:02:12.38 +12:06:06.2
05:55:30.15 +15:07:43.0
06:38:24.91 +16:31:42.9
06:07:05.39 +10:57:47.3
06:12:20.08 +10:02:02.9
06:01:14.33 +14:32:07.9
05:49:53.50 +12:29:45.4
06:02:09.67 +12:11:04.5
06:17:55.26 +14:42:53.9
06:17:02.23 +15:48:27.1
06:20:26.34 +17:59:04.0
06:15:57.83 +15:45:45.1
05:51:24.63 +13:40:34.6
06:31:29.54 +15:00:32.2
05:54:03.01 +13:05:40.2
05:52:22.26 +14:25:29.3
05:54:02.77 +14:48:32.4
06:37:48.45 +13:57:17.5
05:55:31.00 +15:11:03.4
06:03:54.47 +12:44:04.2
06:03:24.37 +14:38:53.9
06:00:15.12 +10:00:43.1
06:38:17.59 +13:56:19.0
06:28:19.35 +16:19:07.2
06:15:53.67 +14:10:16.5
06:25:36.63 +13:37:50.3
05:57:33.47 +10:55:27.7
06:00:12.83 +10:48:38.6
06:32:24.25 +14:54:07.7
06:09:12.73 +15:40:26.2
06:41:18.37 +18:02:06.5
06:11:23.67 +14:49:43.8
05:50:05.21 +10:34:52.9
05:52:18.21 +15:51:58.5
06:13:49.71 +12:47:05.9
06:16:19.10 +12:58:42.3
06:12:48.01 +15:57:44.1
06:32:06.16 +18:09:36.7
05:59:04.15 +15:40:37.4
06:41:47.79 +16:51:34.7
05:58:02.29 +16:49:20.9
06:36:42.85 +11:12:37.7
05:57:29.14 +16:25:49.5
05:57:55.44 +13:34:11.1
06:38:09.24 +15:02:40.6
06:20:24.74 +14:14:42.3
05:52:33.54 +15:43:51.8
06:06:40.77 +15:11:24.5
06:13:23.70 +17:13:26.2
05:51:05.92 +15:39:54.3
06:00:36.43 +11:03:23.1
06:21:53.66 +13:08:31.1
06:26:36.79 +17:47:21.8
06:40:09.43 +14:33:37.8
05:55:57.23 +16:32:15.4
05:56:51.70 +12:21:05.0
06:17:44.87 +14:40:48.6
06:21:40.48 +17:48:04.2
05:48:32.31 +11:28:52.5
06:13:17.34 +11:55:02.2
06:11:10.67 +17:30:32.5
06:26:25.39 +17:42:20.4
05:56:53.22 +14:50:24.1
06:03:45.62 +14:20:46.8
06:16:27.35 +16:42:37.0
06:10:11.93 +17:42:34.7
06:05:20.88 +15:10:13.7
06:19:42.37 +15:59:26.5
05:57:13.85 +17:30:31.4
05:57:47.55 +14:19:56.9
06:35:06.81 +12:37:59.2
06:13:39.25 +12:47:36.1
06:17:11.07 +15:50:13.9
06:06:57.44 +18:07:52.5
05:58:23.29 +14:59:59.7
05:56:44.03 +17:00:10.6
06:22:11.59 +16:05:21.9
06:10:30.86 +14:52:41.5
06:09:52.24 +11:19:55.9
06:36:13.58 +13:05:53.3
06:08:14.29 +13:57:07.0
06:17:52.57 +15:42:08.5
06:23:30.72 +15:36:13.9
06:15:00.70 +14:58:53.8
06:00:20.50 +15:32:27.3
06:18:18.07 +14:22:18.5
06:01:23.34 +13:54:28.3
06:14:42.27 +15:10:59.3
06:25:09.40 +15:58:53.2
06:12:57.12 +17:26:20.8
05:59:57.47 +13:03:23.9
06:14:37.19 +16:02:30.0
06:26:56.70 +16:47:33.6
06:07:01.07 +10:58:45.7
06:22:17.55 +14:40:26.2
05:53:52.19 +10:13:57.5
05:49:29.16 +13:54:40.7
06:12:28.12 +15:20:04.0
06:11:37.12 +15:28:25.8
05:52:38.40 +15:49:35.6
06:12:18.14 +15:12:21.6
05:58:27.75 +14:56:55.0
06:34:47.10 +15:31:02.4
06:00:02.61 +11:09:52.3
06:00:51.40 +10:59:28.2
06:19:47.12 +16:38:52.2
05:52:46.77 +15:24:02.9
06:11:09.03 +17:31:03.4
06:17:01.32 +18:06:38.1
06:12:21.10 +15:28:31.8
06:27:16.30 +15:59:50.2
06:16:19.71 +14:31:17.4
06:21:47.10 +17:02:50.5
05:50:50.22 +14:25:30.8
06:13:44.01 +14:52:17.4
05:57:13.85 +17:08:13.1
06:15:27.96 +14:23:53.8
05:52:19.39 +15:41:14.0
06:19:12.08 +12:45:05.6
06:06:58.48 +14:36:07.6
06:18:12.86 +17:18:43.0
06:27:44.20 +17:39:44.9
06:14:33.77 +14:45:32.8
06:03:52.31 +14:59:06.2
06:27:05.36 +15:18:40.6
06:25:36.83 +14:06:33.7
05:59:07.20 +15:23:10.3
06:12:31.19 +15:20:14.8
06:12:58.78 +16:22:06.4
06:26:01.08 +16:39:51.4
06:17:50.72 +16:23:57.8
05:58:48.36 +13:38:12.1
06:14:14.15 +13:14:59.7
05:48:08.74 +15:56:46.3
05:54:30.48 +12:57:31.2
05:57:54.95 +15:49:12.1
06:18:54.39 +11:33:58.2
06:03:20.61 +10:39:27.7
06:00:57.41 +16:27:52.0
05:56:21.71 +17:58:16.1
05:56:34.56 +10:29:34.4
06:33:00.95 +16:03:44.3
05:51:00.51 +13:29:08.8
06:02:23.83 +16:35:57.0
06:11:05.92 +16:19:10.0
05:55:47.19 +14:48:03.3
06:13:31.18 +17:23:07.5
05:57:00.08 +17:55:39.2
06:09:55.61 +14:26:05.8
06:14:08.40 +17:22:59.2
05:55:13.00 +12:41:16.7
06:20:58.44 +14:41:23.0
06:20:57.41 +16:50:14.0
06:27:51.97 +16:41:06.2
06:19:32.57 +13:26:12.2
05:53:13.24 +14:40:26.3
06:14:22.25 +10:07:40.1
05:49:14.22 +14:41:49.9
05:50:03.76 +10:24:30.6
06:12:26.70 +15:00:24.6
06:01:37.68 +14:43:11.4
06:14:35.97 +13:49:52.3
06:06:48.48 +16:40:37.7
06:05:37.22 +17:10:44.5
06:18:28.69 +14:20:27.4
06:08:55.81 +17:07:39.8
05:55:56.50 +14:38:13.7
06:17:35.47 +14:21:38.3
05:49:16.39 +11:26:25.1
06:15:10.86 +14:43:50.2
06:18:34.84 +14:20:07.9
06:09:57.09 +16:59:12.5
05:58:48.37 +16:29:35.8
06:36:15.89 +17:59:27.2
06:10:46.63 +14:47:20.1
05:57:33.70 +15:38:37.6
06:00:21.97 +10:05:26.5
06:02:09.43 +13:56:17.9
06:00:57.68 +14:31:57.1
06:20:46.73 +15:42:08.3
06:06:05.15 +13:21:02.3
06:23:30.13 +11:14:21.5
05:58:26.36 +15:59:27.8
06:15:37.99 +17:53:12.9
06:17:24.85 +10:19:34.6
05:58:07.30 +16:38:48.8
05:48:53.13 +10:13:09.1
06:10:25.45 +13:28:04.0
05:49:28.19 +11:30:41.1
06:05:57.84 +11:37:35.4
06:19:04.36 +16:47:19.7
06:16:58.67 +18:09:12.6
06:11:38.99 +15:16:52.1
06:04:28.03 +16:29:14.2
06:21:31.34 +14:40:25.4
06:00:15.39 +12:08:18.0
05:57:29.86 +16:51:07.0
06:17:27.80 +11:05:42.3
06:06:00.97 +16:53:36.4
06:25:33.68 +17:35:13.7
05:56:04.67 +16:54:40.0
05:59:56.19 +11:30:34.1
06:17:11.51 +12:04:06.2
06:23:49.20 +16:28:13.7
05:50:25.64 +14:39:13.4
05:59:14.49 +14:14:26.2
06:11:59.01 +17:22:43.5
06:06:48.49 +16:49:38.2
06:24:49.25 +16:41:34.4
06:04:31.59 +15:26:09.2
06:14:21.65 +14:20:39.0
06:14:07.62 +18:00:35.7
06:01:42.11 +16:14:30.9
06:20:01.74 +13:52:51.3
06:04:26.30 +18:02:07.7
06:25:04.23 +16:36:40.2
06:01:19.48 +15:34:36.6
05:58:27.76 +15:59:40.1
06:10:54.56 +14:51:53.8
05:59:32.63 +13:11:26.7
06:18:42.41 +17:53:58.5
06:19:02.13 +16:47:08.0
05:56:16.27 +12:14:41.5
05:51:31.58 +15:47:51.0
06:20:39.35 +13:04:20.9
06:15:27.39 +14:45:49.8
05:57:29.25 +10:49:42.8
06:10:28.12 +13:50:01.6
05:50:15.64 +13:10:20.9
06:13:50.81 +14:44:31.5
06:07:09.40 +16:42:46.9
06:25:46.57 +17:09:24.5
05:59:11.19 +16:41:15.8
06:26:02.09 +15:47:59.3
05:58:52.27 +13:37:22.3
05:51:44.60 +15:34:43.5
05:51:19.82 +13:57:03.9
06:13:47.44 +15:24:03.1
06:16:28.87 +15:12:39.8
06:01:20.72 +17:26:15.5
05:55:50.23 +17:41:16.2
06:20:42.81 +17:46:45.8
06:19:59.21 +17:10:05.3
05:52:03.63 +15:17:57.9
05:52:24.06 +13:07:42.1
05:57:35.03 +15:59:00.1
05:57:42.27 +15:57:13.2
06:02:07.56 +15:11:23.2
06:13:10.18 +12:55:19.3
05:59:54.48 +16:54:38.7
06:19:36.57 +17:40:29.3
06:20:16.95 +13:20:08.4
05:55:56.82 +17:18:04.4
05:55:03.80 +15:54:25.8
05:58:30.34 +17:44:47.9
05:57:06.30 +17:40:03.3
06:27:31.25 +15:16:12.9
05:50:07.25 +15:27:57.1
05:56:47.22 +17:56:00.9
06:04:09.22 +15:25:54.2
05:57:37.01 +16:32:37.8
06:18:00.48 +17:37:01.4
05:48:37.32 +15:50:58.7
05:51:06.30 +15:03:04.4
05:56:09.13 +17:46:33.2
06:05:46.85 +10:58:59.2
06:02:07.79 +16:23:46.6
06:06:25.19 +16:38:04.6
05:55:23.29 +14:46:09.8
05:54:30.03 +14:48:43.8
05:51:14.90 +14:02:32.7
06:20:35.52 +13:38:05.2
05:56:33.13 +15:24:54.7
06:18:21.39 +17:01:39.7
05:59:25.67 +15:07:24.7
05:56:40.30 +16:06:18.8
06:01:21.00 +12:23:32.8
06:09:30.91 +13:08:59.7
05:59:57.80 +17:18:57.4
05:50:27.70 +15:04:18.3
05:53:11.70 +14:46:13.7
06:18:51.02 +14:40:00.2
05:56:00.89 +15:07:20.7
06:21:30.97 +15:43:18.3
06:10:55.00 +17:26:53.0
06:15:16.16 +15:59:57.2
05:49:48.99 +11:48:49.0
06:21:23.34 +13:14:45.8
05:58:23.72 +11:50:43.1
###################################################################################
06:35:44.72 +11:17:02.2 -- asteroid (will NOT add it to exclusion list)
06:04:11.35 +12:35:21.9 -- not an asteroid (will add it to exclusion list)
06:14:35.48 +11:15:30.7 -- not an asteroid (will add it to exclusion list)
06:01:33.03 +12:58:52.5 -- not an asteroid (will add it to exclusion list)
06:13:19.53 +14:42:59.0 -- not an asteroid (will add it to exclusion list)
06:11:39.40 +15:01:29.1 -- not an asteroid (will add it to exclusion list)
06:00:51.32 +16:19:51.9 -- not an asteroid (will add it to exclusion list)
06:08:32.34 +12:55:13.0 -- not an asteroid (will add it to exclusion list)
06:15:54.44 +12:55:37.6 -- not an asteroid (will add it to exclusion list)
05:58:30.36 +17:12:37.4 -- not an asteroid (will add it to exclusion list)
05:58:29.54 +15:03:34.6 -- not an asteroid (will add it to exclusion list)
06:28:29.58 +15:24:33.8 -- not an asteroid (will add it to exclusion list)
06:11:23.33 +15:36:18.7 -- not an asteroid (will add it to exclusion list)
06:11:51.37 +15:43:45.7 -- not an asteroid (will add it to exclusion list)
05:56:00.70 +11:46:10.3 -- not an asteroid (will add it to exclusion list)
06:08:22.48 +11:49:59.2 -- not an asteroid (will add it to exclusion list)
05:50:15.94 +13:54:06.7 -- not an asteroid (will add it to exclusion list)
06:11:31.89 +13:26:07.7 -- not an asteroid (will add it to exclusion list)
06:32:37.70 +17:57:41.0 -- not an asteroid (will add it to exclusion list)
05:50:13.32 +13:10:47.3 -- not an asteroid (will add it to exclusion list)
05:52:57.06 +13:18:07.9 -- not an asteroid (will add it to exclusion list)
06:01:37.27 +15:19:51.9 -- not an asteroid (will add it to exclusion list)
06:01:45.31 +11:15:08.8 -- not an asteroid (will add it to exclusion list)
06:02:38.41 +14:07:58.5 -- not an asteroid (will add it to exclusion list)
06:31:46.63 +18:03:22.1 -- not an asteroid (will add it to exclusion list)
06:06:13.09 +16:19:25.9 -- not an asteroid (will add it to exclusion list)
05:59:02.80 +14:46:12.3 -- not an asteroid (will add it to exclusion list)
06:02:21.36 +16:12:34.2 -- not an asteroid (will add it to exclusion list)
06:08:27.07 +16:23:02.2 -- not an asteroid (will add it to exclusion list)
06:30:27.64 +13:42:19.9 -- not an asteroid (will add it to exclusion list)
05:55:28.40 +12:46:35.7 -- not an asteroid (will add it to exclusion list)
05:55:21.77 +15:39:09.2 -- not an asteroid (will add it to exclusion list)
06:04:18.72 +12:32:52.4 -- not an asteroid (will add it to exclusion list)
06:09:52.59 +14:42:45.0 -- not an asteroid (will add it to exclusion list)
05:52:23.63 +14:54:07.5 -- not an asteroid (will add it to exclusion list)
06:26:01.11 +16:56:24.1 -- not an asteroid (will add it to exclusion list)
06:10:22.29 +16:14:32.2 -- not an asteroid (will add it to exclusion list)
06:34:28.25 +17:43:05.2 -- not an asteroid (will add it to exclusion list)
06:01:12.93 +14:02:43.4 -- not an asteroid (will add it to exclusion list)
06:00:38.09 +15:37:19.4 -- not an asteroid (will add it to exclusion list)
06:31:42.38 +16:47:43.8 -- not an asteroid (will add it to exclusion list)
06:00:38.27 +15:56:45.7 -- not an asteroid (will add it to exclusion list)
06:11:44.51 +17:21:10.0 -- not an asteroid (will add it to exclusion list)
06:27:07.91 +16:55:02.4 -- not an asteroid (will add it to exclusion list)
05:57:44.30 +13:34:32.9 -- not an asteroid (will add it to exclusion list)
06:21:43.42 +12:44:20.6 -- not an asteroid (will add it to exclusion list)
05:51:44.66 +14:17:01.2 -- not an asteroid (will add it to exclusion list)
06:07:08.68 +12:32:31.1 -- not an asteroid (will add it to exclusion list)
06:08:08.26 +14:27:05.4 -- not an asteroid (will add it to exclusion list)
06:15:50.94 +17:58:52.8 -- not an asteroid (will add it to exclusion list)
05:57:00.12 +13:28:56.6 -- not an asteroid (will add it to exclusion list)
06:15:32.34 +13:47:36.2 -- not an asteroid (will add it to exclusion list)
06:13:27.53 +14:13:51.9 -- not an asteroid (will add it to exclusion list)
06:10:32.45 +16:29:31.2 -- not an asteroid (will add it to exclusion list)
05:54:18.55 +15:25:19.1 -- not an asteroid (will add it to exclusion list)
05:54:12.38 +15:02:21.1 -- not an asteroid (will add it to exclusion list)
05:57:35.31 +17:58:56.7 -- not an asteroid (will add it to exclusion list)
06:02:12.38 +12:06:06.2 -- not an asteroid (will add it to exclusion list)
05:55:30.15 +15:07:43.0 -- not an asteroid (will add it to exclusion list)
06:38:24.91 +16:31:42.9 -- not an asteroid (will add it to exclusion list)
06:07:05.39 +10:57:47.3 -- not an asteroid (will add it to exclusion list)
06:12:20.08 +10:02:02.9 -- not an asteroid (will add it to exclusion list)
06:01:14.33 +14:32:07.9 -- not an asteroid (will add it to exclusion list)
05:49:53.50 +12:29:45.4 -- not an asteroid (will add it to exclusion list)
06:02:09.67 +12:11:04.5 -- not an asteroid (will add it to exclusion list)
06:17:55.26 +14:42:53.9 -- not an asteroid (will add it to exclusion list)
06:17:02.23 +15:48:27.1 -- not an asteroid (will add it to exclusion list)
06:20:26.34 +17:59:04.0 -- not an asteroid (will add it to exclusion list)
06:15:57.83 +15:45:45.1 -- not an asteroid (will add it to exclusion list)
05:51:24.63 +13:40:34.6 -- not an asteroid (will add it to exclusion list)
06:31:29.54 +15:00:32.2 -- not an asteroid (will add it to exclusion list)
05:54:03.01 +13:05:40.2 -- not an asteroid (will add it to exclusion list)
05:52:22.26 +14:25:29.3 -- not an asteroid (will add it to exclusion list)
05:54:02.77 +14:48:32.4 -- not an asteroid (will add it to exclusion list)
06:37:48.45 +13:57:17.5 -- not an asteroid (will add it to exclusion list)
05:55:31.00 +15:11:03.4 -- not an asteroid (will add it to exclusion list)
06:03:54.47 +12:44:04.2 -- not an asteroid (will add it to exclusion list)
06:03:24.37 +14:38:53.9 -- not an asteroid (will add it to exclusion list)
06:00:15.12 +10:00:43.1 -- asteroid (will NOT add it to exclusion list)
06:38:17.59 +13:56:19.0 -- not an asteroid (will add it to exclusion list)
06:28:19.35 +16:19:07.2 -- not an asteroid (will add it to exclusion list)
06:15:53.67 +14:10:16.5 -- not an asteroid (will add it to exclusion list)
06:25:36.63 +13:37:50.3 -- not an asteroid (will add it to exclusion list)
05:57:33.47 +10:55:27.7 -- not an asteroid (will add it to exclusion list)
06:00:12.83 +10:48:38.6 -- not an asteroid (will add it to exclusion list)
06:32:24.25 +14:54:07.7 -- not an asteroid (will add it to exclusion list)
06:09:12.73 +15:40:26.2 -- not an asteroid (will add it to exclusion list)
06:41:18.37 +18:02:06.5 -- not an asteroid (will add it to exclusion list)
06:11:23.67 +14:49:43.8 -- not an asteroid (will add it to exclusion list)
05:50:05.21 +10:34:52.9 -- not an asteroid (will add it to exclusion list)
05:52:18.21 +15:51:58.5 -- not an asteroid (will add it to exclusion list)
06:13:49.71 +12:47:05.9 -- not an asteroid (will add it to exclusion list)
06:16:19.10 +12:58:42.3 -- not an asteroid (will add it to exclusion list)
06:12:48.01 +15:57:44.1 -- not an asteroid (will add it to exclusion list)
06:32:06.16 +18:09:36.7 -- not an asteroid (will add it to exclusion list)
05:59:04.15 +15:40:37.4 -- not an asteroid (will add it to exclusion list)
06:41:47.79 +16:51:34.7 -- not an asteroid (will add it to exclusion list)
05:58:02.29 +16:49:20.9 -- not an asteroid (will add it to exclusion list)
06:36:42.85 +11:12:37.7 -- not an asteroid (will add it to exclusion list)
05:57:29.14 +16:25:49.5 -- not an asteroid (will add it to exclusion list)
05:57:55.44 +13:34:11.1 -- not an asteroid (will add it to exclusion list)
06:38:09.24 +15:02:40.6 -- not an asteroid (will add it to exclusion list)
06:20:24.74 +14:14:42.3 -- not an asteroid (will add it to exclusion list)
05:52:33.54 +15:43:51.8 -- not an asteroid (will add it to exclusion list)
06:06:40.77 +15:11:24.5 -- not an asteroid (will add it to exclusion list)
06:13:23.70 +17:13:26.2 -- not an asteroid (will add it to exclusion list)
05:51:05.92 +15:39:54.3 -- not an asteroid (will add it to exclusion list)
06:00:36.43 +11:03:23.1 -- not an asteroid (will add it to exclusion list)
06:21:53.66 +13:08:31.1 -- not an asteroid (will add it to exclusion list)
06:26:36.79 +17:47:21.8 -- not an asteroid (will add it to exclusion list)
06:40:09.43 +14:33:37.8 -- not an asteroid (will add it to exclusion list)
05:55:57.23 +16:32:15.4 -- not an asteroid (will add it to exclusion list)
05:56:51.70 +12:21:05.0 -- not an asteroid (will add it to exclusion list)
06:17:44.87 +14:40:48.6 -- not an asteroid (will add it to exclusion list)
06:21:40.48 +17:48:04.2 -- not an asteroid (will add it to exclusion list)
05:48:32.31 +11:28:52.5 -- not an asteroid (will add it to exclusion list)
06:13:17.34 +11:55:02.2 -- not an asteroid (will add it to exclusion list)
06:11:10.67 +17:30:32.5 -- not an asteroid (will add it to exclusion list)
06:26:25.39 +17:42:20.4 -- not an asteroid (will add it to exclusion list)
05:56:53.22 +14:50:24.1 -- asteroid (will NOT add it to exclusion list)
06:03:45.62 +14:20:46.8 -- not an asteroid (will add it to exclusion list)
06:16:27.35 +16:42:37.0 -- not an asteroid (will add it to exclusion list)
06:10:11.93 +17:42:34.7 -- not an asteroid (will add it to exclusion list)
06:05:20.88 +15:10:13.7 -- not an asteroid (will add it to exclusion list)
06:19:42.37 +15:59:26.5 -- not an asteroid (will add it to exclusion list)
05:57:13.85 +17:30:31.4 -- not an asteroid (will add it to exclusion list)
05:57:47.55 +14:19:56.9 -- asteroid (will NOT add it to exclusion list)
06:35:06.81 +12:37:59.2 -- not an asteroid (will add it to exclusion list)
06:13:39.25 +12:47:36.1 -- not an asteroid (will add it to exclusion list)
06:17:11.07 +15:50:13.9 -- not an asteroid (will add it to exclusion list)
06:06:57.44 +18:07:52.5 -- not an asteroid (will add it to exclusion list)
05:58:23.29 +14:59:59.7 -- not an asteroid (will add it to exclusion list)
05:56:44.03 +17:00:10.6 -- not an asteroid (will add it to exclusion list)
06:22:11.59 +16:05:21.9 -- not an asteroid (will add it to exclusion list)
06:10:30.86 +14:52:41.5 -- not an asteroid (will add it to exclusion list)
06:09:52.24 +11:19:55.9 -- not an asteroid (will add it to exclusion list)
06:36:13.58 +13:05:53.3 -- not an asteroid (will add it to exclusion list)
06:08:14.29 +13:57:07.0 -- not an asteroid (will add it to exclusion list)
06:17:52.57 +15:42:08.5 -- not an asteroid (will add it to exclusion list)
06:23:30.72 +15:36:13.9 -- not an asteroid (will add it to exclusion list)
06:15:00.70 +14:58:53.8 -- not an asteroid (will add it to exclusion list)
06:00:20.50 +15:32:27.3 -- not an asteroid (will add it to exclusion list)
06:18:18.07 +14:22:18.5 -- not an asteroid (will add it to exclusion list)
06:01:23.34 +13:54:28.3 -- not an asteroid (will add it to exclusion list)
06:14:42.27 +15:10:59.3 -- not an asteroid (will add it to exclusion list)
06:25:09.40 +15:58:53.2 -- not an asteroid (will add it to exclusion list)
06:12:57.12 +17:26:20.8 -- not an asteroid (will add it to exclusion list)
05:59:57.47 +13:03:23.9 -- not an asteroid (will add it to exclusion list)
06:14:37.19 +16:02:30.0 -- not an asteroid (will add it to exclusion list)
06:26:56.70 +16:47:33.6 -- not an asteroid (will add it to exclusion list)
06:07:01.07 +10:58:45.7 -- not an asteroid (will add it to exclusion list)
06:22:17.55 +14:40:26.2 -- not an asteroid (will add it to exclusion list)
05:53:52.19 +10:13:57.5 -- not an asteroid (will add it to exclusion list)
05:49:29.16 +13:54:40.7 -- not an asteroid (will add it to exclusion list)
06:12:28.12 +15:20:04.0 -- not an asteroid (will add it to exclusion list)
06:11:37.12 +15:28:25.8 -- not an asteroid (will add it to exclusion list)
05:52:38.40 +15:49:35.6 -- not an asteroid (will add it to exclusion list)
06:12:18.14 +15:12:21.6 -- not an asteroid (will add it to exclusion list)
05:58:27.75 +14:56:55.0 -- not an asteroid (will add it to exclusion list)
06:34:47.10 +15:31:02.4 -- not an asteroid (will add it to exclusion list)
06:00:02.61 +11:09:52.3 -- not an asteroid (will add it to exclusion list)
06:00:51.40 +10:59:28.2 -- not an asteroid (will add it to exclusion list)
06:19:47.12 +16:38:52.2 -- not an asteroid (will add it to exclusion list)
05:52:46.77 +15:24:02.9 -- not an asteroid (will add it to exclusion list)
06:11:09.03 +17:31:03.4 -- not an asteroid (will add it to exclusion list)
06:17:01.32 +18:06:38.1 -- not an asteroid (will add it to exclusion list)
06:12:21.10 +15:28:31.8 -- not an asteroid (will add it to exclusion list)
06:27:16.30 +15:59:50.2 -- not an asteroid (will add it to exclusion list)
06:16:19.71 +14:31:17.4 -- not an asteroid (will add it to exclusion list)
06:21:47.10 +17:02:50.5 -- not an asteroid (will add it to exclusion list)
05:50:50.22 +14:25:30.8 -- not an asteroid (will add it to exclusion list)
06:13:44.01 +14:52:17.4 -- not an asteroid (will add it to exclusion list)
05:57:13.85 +17:08:13.1 -- not an asteroid (will add it to exclusion list)
06:15:27.96 +14:23:53.8 -- not an asteroid (will add it to exclusion list)
05:52:19.39 +15:41:14.0 -- not an asteroid (will add it to exclusion list)
06:19:12.08 +12:45:05.6 -- not an asteroid (will add it to exclusion list)
06:06:58.48 +14:36:07.6 -- not an asteroid (will add it to exclusion list)
06:18:12.86 +17:18:43.0 -- not an asteroid (will add it to exclusion list)
06:27:44.20 +17:39:44.9 -- not an asteroid (will add it to exclusion list)
06:14:33.77 +14:45:32.8 -- not an asteroid (will add it to exclusion list)
06:03:52.31 +14:59:06.2 -- not an asteroid (will add it to exclusion list)
06:27:05.36 +15:18:40.6 -- not an asteroid (will add it to exclusion list)
06:25:36.83 +14:06:33.7 -- not an asteroid (will add it to exclusion list)
05:59:07.20 +15:23:10.3 -- not an asteroid (will add it to exclusion list)
06:12:31.19 +15:20:14.8 -- not an asteroid (will add it to exclusion list)
06:12:58.78 +16:22:06.4 -- not an asteroid (will add it to exclusion list)
06:26:01.08 +16:39:51.4 -- not an asteroid (will add it to exclusion list)
06:17:50.72 +16:23:57.8 -- not an asteroid (will add it to exclusion list)
05:58:48.36 +13:38:12.1 -- not an asteroid (will add it to exclusion list)
06:14:14.15 +13:14:59.7 -- not an asteroid (will add it to exclusion list)
05:48:08.74 +15:56:46.3 -- not an asteroid (will add it to exclusion list)
05:54:30.48 +12:57:31.2 -- not an asteroid (will add it to exclusion list)
05:57:54.95 +15:49:12.1 -- not an asteroid (will add it to exclusion list)
06:18:54.39 +11:33:58.2 -- not an asteroid (will add it to exclusion list)
06:03:20.61 +10:39:27.7 -- not an asteroid (will add it to exclusion list)
06:00:57.41 +16:27:52.0 -- not an asteroid (will add it to exclusion list)
05:56:21.71 +17:58:16.1 -- not an asteroid (will add it to exclusion list)
05:56:34.56 +10:29:34.4 -- not an asteroid (will add it to exclusion list)
06:33:00.95 +16:03:44.3 -- not an asteroid (will add it to exclusion list)
05:51:00.51 +13:29:08.8 -- not an asteroid (will add it to exclusion list)
06:02:23.83 +16:35:57.0 -- not an asteroid (will add it to exclusion list)
06:11:05.92 +16:19:10.0 -- not an asteroid (will add it to exclusion list)
05:55:47.19 +14:48:03.3 -- not an asteroid (will add it to exclusion list)
06:13:31.18 +17:23:07.5 -- not an asteroid (will add it to exclusion list)
05:57:00.08 +17:55:39.2 -- not an asteroid (will add it to exclusion list)
06:09:55.61 +14:26:05.8 -- not an asteroid (will add it to exclusion list)
06:14:08.40 +17:22:59.2 -- not an asteroid (will add it to exclusion list)
05:55:13.00 +12:41:16.7 -- not an asteroid (will add it to exclusion list)
06:20:58.44 +14:41:23.0 -- not an asteroid (will add it to exclusion list)
06:20:57.41 +16:50:14.0 -- not an asteroid (will add it to exclusion list)
06:27:51.97 +16:41:06.2 -- not an asteroid (will add it to exclusion list)
06:19:32.57 +13:26:12.2 -- not an asteroid (will add it to exclusion list)
05:53:13.24 +14:40:26.3 -- not an asteroid (will add it to exclusion list)
06:14:22.25 +10:07:40.1 -- not an asteroid (will add it to exclusion list)
05:49:14.22 +14:41:49.9 -- not an asteroid (will add it to exclusion list)
05:50:03.76 +10:24:30.6 -- not an asteroid (will add it to exclusion list)
06:12:26.70 +15:00:24.6 -- not an asteroid (will add it to exclusion list)
06:01:37.68 +14:43:11.4 -- not an asteroid (will add it to exclusion list)
06:14:35.97 +13:49:52.3 -- not an asteroid (will add it to exclusion list)
06:06:48.48 +16:40:37.7 -- not an asteroid (will add it to exclusion list)
06:05:37.22 +17:10:44.5 -- not an asteroid (will add it to exclusion list)
06:18:28.69 +14:20:27.4 -- not an asteroid (will add it to exclusion list)
06:08:55.81 +17:07:39.8 -- not an asteroid (will add it to exclusion list)
05:55:56.50 +14:38:13.7 -- not an asteroid (will add it to exclusion list)
06:17:35.47 +14:21:38.3 -- not an asteroid (will add it to exclusion list)
05:49:16.39 +11:26:25.1 -- not an asteroid (will add it to exclusion list)
06:15:10.86 +14:43:50.2 -- not an asteroid (will add it to exclusion list)
06:18:34.84 +14:20:07.9 -- not an asteroid (will add it to exclusion list)
06:09:57.09 +16:59:12.5 -- not an asteroid (will add it to exclusion list)
05:58:48.37 +16:29:35.8 -- not an asteroid (will add it to exclusion list)
06:36:15.89 +17:59:27.2 -- not an asteroid (will add it to exclusion list)
06:10:46.63 +14:47:20.1 -- not an asteroid (will add it to exclusion list)
05:57:33.70 +15:38:37.6 -- not an asteroid (will add it to exclusion list)
06:00:21.97 +10:05:26.5 -- asteroid (will NOT add it to exclusion list)
06:02:09.43 +13:56:17.9 -- not an asteroid (will add it to exclusion list)
06:00:57.68 +14:31:57.1 -- not an asteroid (will add it to exclusion list)
06:20:46.73 +15:42:08.3 -- not an asteroid (will add it to exclusion list)
06:06:05.15 +13:21:02.3 -- not an asteroid (will add it to exclusion list)
06:23:30.13 +11:14:21.5 -- not an asteroid (will add it to exclusion list)
05:58:26.36 +15:59:27.8 -- not an asteroid (will add it to exclusion list)
06:15:37.99 +17:53:12.9 -- not an asteroid (will add it to exclusion list)
06:17:24.85 +10:19:34.6 -- not an asteroid (will add it to exclusion list)
05:58:07.30 +16:38:48.8 -- not an asteroid (will add it to exclusion list)
05:48:53.13 +10:13:09.1 -- not an asteroid (will add it to exclusion list)
06:10:25.45 +13:28:04.0 -- not an asteroid (will add it to exclusion list)
05:49:28.19 +11:30:41.1 -- not an asteroid (will add it to exclusion list)
06:05:57.84 +11:37:35.4 -- not an asteroid (will add it to exclusion list)
06:19:04.36 +16:47:19.7 -- not an asteroid (will add it to exclusion list)
06:16:58.67 +18:09:12.6 -- not an asteroid (will add it to exclusion list)
06:11:38.99 +15:16:52.1 -- not an asteroid (will add it to exclusion list)
06:04:28.03 +16:29:14.2 -- not an asteroid (will add it to exclusion list)
06:21:31.34 +14:40:25.4 -- not an asteroid (will add it to exclusion list)
06:00:15.39 +12:08:18.0 -- not an asteroid (will add it to exclusion list)
05:57:29.86 +16:51:07.0 -- not an asteroid (will add it to exclusion list)
06:17:27.80 +11:05:42.3 -- asteroid (will NOT add it to exclusion list)
06:06:00.97 +16:53:36.4 -- not an asteroid (will add it to exclusion list)
06:25:33.68 +17:35:13.7 -- not an asteroid (will add it to exclusion list)
05:56:04.67 +16:54:40.0 -- not an asteroid (will add it to exclusion list)
05:59:56.19 +11:30:34.1 -- not an asteroid (will add it to exclusion list)
06:17:11.51 +12:04:06.2 -- not an asteroid (will add it to exclusion list)
06:23:49.20 +16:28:13.7 -- not an asteroid (will add it to exclusion list)
05:50:25.64 +14:39:13.4 -- asteroid (will NOT add it to exclusion list)
05:59:14.49 +14:14:26.2 -- not an asteroid (will add it to exclusion list)
06:11:59.01 +17:22:43.5 -- not an asteroid (will add it to exclusion list)
06:06:48.49 +16:49:38.2 -- not an asteroid (will add it to exclusion list)
06:24:49.25 +16:41:34.4 -- not an asteroid (will add it to exclusion list)
06:04:31.59 +15:26:09.2 -- not an asteroid (will add it to exclusion list)
06:14:21.65 +14:20:39.0 -- not an asteroid (will add it to exclusion list)
06:14:07.62 +18:00:35.7 -- not an asteroid (will add it to exclusion list)
06:01:42.11 +16:14:30.9 -- not an asteroid (will add it to exclusion list)
06:20:01.74 +13:52:51.3 -- not an asteroid (will add it to exclusion list)
06:04:26.30 +18:02:07.7 -- not an asteroid (will add it to exclusion list)
06:25:04.23 +16:36:40.2 -- not an asteroid (will add it to exclusion list)
06:01:19.48 +15:34:36.6 -- not an asteroid (will add it to exclusion list)
05:58:27.76 +15:59:40.1 -- not an asteroid (will add it to exclusion list)
06:10:54.56 +14:51:53.8 -- not an asteroid (will add it to exclusion list)
05:59:32.63 +13:11:26.7 -- not an asteroid (will add it to exclusion list)
06:18:42.41 +17:53:58.5 -- not an asteroid (will add it to exclusion list)
06:19:02.13 +16:47:08.0 -- not an asteroid (will add it to exclusion list)
05:56:16.27 +12:14:41.5 -- not an asteroid (will add it to exclusion list)
05:51:31.58 +15:47:51.0 -- not an asteroid (will add it to exclusion list)
06:20:39.35 +13:04:20.9 -- not an asteroid (will add it to exclusion list)
06:15:27.39 +14:45:49.8 -- not an asteroid (will add it to exclusion list)
05:57:29.25 +10:49:42.8 -- not an asteroid (will add it to exclusion list)
06:10:28.12 +13:50:01.6 -- not an asteroid (will add it to exclusion list)
05:50:15.64 +13:10:20.9 -- not an asteroid (will add it to exclusion list)
06:13:50.81 +14:44:31.5 -- not an asteroid (will add it to exclusion list)
06:07:09.40 +16:42:46.9 -- not an asteroid (will add it to exclusion list)
06:25:46.57 +17:09:24.5 -- not an asteroid (will add it to exclusion list)
05:59:11.19 +16:41:15.8 -- not an asteroid (will add it to exclusion list)
06:26:02.09 +15:47:59.3 -- not an asteroid (will add it to exclusion list)
05:58:52.27 +13:37:22.3 -- not an asteroid (will add it to exclusion list)
05:51:44.60 +15:34:43.5 -- not an asteroid (will add it to exclusion list)
05:51:19.82 +13:57:03.9 -- not an asteroid (will add it to exclusion list)
06:13:47.44 +15:24:03.1 -- not an asteroid (will add it to exclusion list)
06:16:28.87 +15:12:39.8 -- not an asteroid (will add it to exclusion list)
06:01:20.72 +17:26:15.5 -- not an asteroid (will add it to exclusion list)
05:55:50.23 +17:41:16.2 -- not an asteroid (will add it to exclusion list)
06:20:42.81 +17:46:45.8 -- not an asteroid (will add it to exclusion list)
06:19:59.21 +17:10:05.3 -- not an asteroid (will add it to exclusion list)
05:52:03.63 +15:17:57.9 -- not an asteroid (will add it to exclusion list)
05:52:24.06 +13:07:42.1 -- not an asteroid (will add it to exclusion list)
05:57:35.03 +15:59:00.1 -- not an asteroid (will add it to exclusion list)
05:57:42.27 +15:57:13.2 -- not an asteroid (will add it to exclusion list)
06:02:07.56 +15:11:23.2 -- not an asteroid (will add it to exclusion list)
06:13:10.18 +12:55:19.3 -- not an asteroid (will add it to exclusion list)
05:59:54.48 +16:54:38.7 -- not an asteroid (will add it to exclusion list)
06:19:36.57 +17:40:29.3 -- not an asteroid (will add it to exclusion list)
06:20:16.95 +13:20:08.4 -- not an asteroid (will add it to exclusion list)
05:55:56.82 +17:18:04.4 -- not an asteroid (will add it to exclusion list)
05:55:03.80 +15:54:25.8 -- not an asteroid (will add it to exclusion list)
05:58:30.34 +17:44:47.9 -- not an asteroid (will add it to exclusion list)
05:57:06.30 +17:40:03.3 -- not an asteroid (will add it to exclusion list)
06:27:31.25 +15:16:12.9 -- not an asteroid (will add it to exclusion list)
05:50:07.25 +15:27:57.1 -- not an asteroid (will add it to exclusion list)
05:56:47.22 +17:56:00.9 -- not an asteroid (will add it to exclusion list)
06:04:09.22 +15:25:54.2 -- not an asteroid (will add it to exclusion list)
05:57:37.01 +16:32:37.8 -- not an asteroid (will add it to exclusion list)
06:18:00.48 +17:37:01.4 -- not an asteroid (will add it to exclusion list)
05:48:37.32 +15:50:58.7 -- not an asteroid (will add it to exclusion list)
05:51:06.30 +15:03:04.4 -- not an asteroid (will add it to exclusion list)
05:56:09.13 +17:46:33.2 -- not an asteroid (will add it to exclusion list)
06:05:46.85 +10:58:59.2 -- not an asteroid (will add it to exclusion list)
06:02:07.79 +16:23:46.6 -- not an asteroid (will add it to exclusion list)
06:06:25.19 +16:38:04.6 -- not an asteroid (will add it to exclusion list)
05:55:23.29 +14:46:09.8 -- not an asteroid (will add it to exclusion list)
05:54:30.03 +14:48:43.8 -- not an asteroid (will add it to exclusion list)
05:51:14.90 +14:02:32.7 -- not an asteroid (will add it to exclusion list)
06:20:35.52 +13:38:05.2 -- not an asteroid (will add it to exclusion list)
05:56:33.13 +15:24:54.7 -- not an asteroid (will add it to exclusion list)
06:18:21.39 +17:01:39.7 -- not an asteroid (will add it to exclusion list)
05:59:25.67 +15:07:24.7 -- not an asteroid (will add it to exclusion list)
05:56:40.30 +16:06:18.8 -- not an asteroid (will add it to exclusion list)
06:01:21.00 +12:23:32.8 -- not an asteroid (will add it to exclusion list)
06:09:30.91 +13:08:59.7 -- not an asteroid (will add it to exclusion list)
05:59:57.80 +17:18:57.4 -- not an asteroid (will add it to exclusion list)
05:50:27.70 +15:04:18.3 -- not an asteroid (will add it to exclusion list)
05:53:11.70 +14:46:13.7 -- not an asteroid (will add it to exclusion list)
06:18:51.02 +14:40:00.2 -- not an asteroid (will add it to exclusion list)
05:56:00.89 +15:07:20.7 -- not an asteroid (will add it to exclusion list)
06:21:30.97 +15:43:18.3 -- not an asteroid (will add it to exclusion list)
06:10:55.00 +17:26:53.0 -- not an asteroid (will add it to exclusion list)
06:15:16.16 +15:59:57.2 -- not an asteroid (will add it to exclusion list)
05:49:48.99 +11:48:49.0 -- not an asteroid (will add it to exclusion list)
06:21:23.34 +13:14:45.8 -- not an asteroid (will add it to exclusion list)
05:58:23.72 +11:50:43.1 -- asteroid (will NOT add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:48:08.74 +15:56:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:32.31 +11:28:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:37.32 +15:50:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.13 +10:13:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:14.22 +14:41:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:16.39 +11:26:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:28.19 +11:30:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:29.16 +13:54:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:48.99 +11:48:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:53.50 +12:29:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:03.76 +10:24:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:05.21 +10:34:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:07.25 +15:27:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:13.32 +13:10:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:15.64 +13:10:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:15.94 +13:54:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:27.70 +15:04:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:50.22 +14:25:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:00.51 +13:29:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:05.92 +15:39:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:06.30 +15:03:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:14.90 +14:02:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:19.82 +13:57:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:24.63 +13:40:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:31.58 +15:47:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:44.60 +15:34:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:44.66 +14:17:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:03.63 +15:17:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:18.21 +15:51:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:19.39 +15:41:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:22.26 +14:25:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:23.63 +14:54:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:24.06 +13:07:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:33.54 +15:43:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:38.40 +15:49:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:46.77 +15:24:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:57.06 +13:18:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:11.70 +14:46:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:13.24 +14:40:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:52.19 +10:13:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:02.77 +14:48:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:03.01 +13:05:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:12.38 +15:02:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:18.55 +15:25:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:30.03 +14:48:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:30.48 +12:57:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:03.80 +15:54:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:13.00 +12:41:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:21.77 +15:39:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:23.29 +14:46:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:28.40 +12:46:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:30.15 +15:07:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:31.00 +15:11:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:47.19 +14:48:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:50.23 +17:41:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:56.50 +14:38:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:56.82 +17:18:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:57.23 +16:32:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:00.70 +11:46:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:00.89 +15:07:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:04.67 +16:54:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:09.13 +17:46:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:16.27 +12:14:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:21.71 +17:58:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:33.13 +15:24:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:34.56 +10:29:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:40.30 +16:06:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:44.03 +17:00:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:47.22 +17:56:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:51.70 +12:21:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:00.08 +17:55:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:00.12 +13:28:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:06.30 +17:40:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:13.85 +17:08:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:13.85 +17:30:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:29.14 +16:25:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:29.25 +10:49:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:29.86 +16:51:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:33.47 +10:55:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:33.70 +15:38:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:35.03 +15:59:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:35.31 +17:58:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:37.01 +16:32:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:42.27 +15:57:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:44.30 +13:34:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:54.95 +15:49:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:55.44 +13:34:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:02.29 +16:49:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:07.30 +16:38:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:23.29 +14:59:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:26.36 +15:59:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:27.75 +14:56:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:27.76 +15:59:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:29.54 +15:03:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:30.34 +17:44:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:30.36 +17:12:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:48.36 +13:38:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:48.37 +16:29:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:52.27 +13:37:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:02.80 +14:46:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:04.15 +15:40:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:07.20 +15:23:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:11.19 +16:41:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:14.49 +14:14:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:25.67 +15:07:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:32.63 +13:11:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:54.48 +16:54:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:56.19 +11:30:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:57.47 +13:03:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:57.80 +17:18:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:02.61 +11:09:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:12.83 +10:48:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:15.39 +12:08:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:20.50 +15:32:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:36.43 +11:03:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:38.09 +15:37:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:38.27 +15:56:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:51.32 +16:19:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:51.40 +10:59:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:57.41 +16:27:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:57.68 +14:31:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:12.93 +14:02:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:14.33 +14:32:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:19.48 +15:34:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:20.72 +17:26:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:21.00 +12:23:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:23.34 +13:54:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:33.03 +12:58:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:37.27 +15:19:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:37.68 +14:43:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:42.11 +16:14:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:45.31 +11:15:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:07.56 +15:11:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:07.79 +16:23:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:09.43 +13:56:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:09.67 +12:11:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:12.38 +12:06:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:21.36 +16:12:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:23.83 +16:35:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:38.41 +14:07:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:20.61 +10:39:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:24.37 +14:38:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:45.62 +14:20:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:52.31 +14:59:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:54.47 +12:44:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:09.22 +15:25:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:11.35 +12:35:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:18.72 +12:32:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:26.30 +18:02:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:28.03 +16:29:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:31.59 +15:26:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:20.88 +15:10:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:37.22 +17:10:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:46.85 +10:58:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:57.84 +11:37:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:00.97 +16:53:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:05.15 +13:21:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:13.09 +16:19:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:25.19 +16:38:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:40.77 +15:11:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:48.48 +16:40:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:48.49 +16:49:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:57.44 +18:07:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:58.48 +14:36:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:01.07 +10:58:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:05.39 +10:57:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:08.68 +12:32:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:09.40 +16:42:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:08.26 +14:27:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:14.29 +13:57:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:22.48 +11:49:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:27.07 +16:23:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:32.34 +12:55:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:55.81 +17:07:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:12.73 +15:40:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:30.91 +13:08:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:52.24 +11:19:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:52.59 +14:42:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:55.61 +14:26:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:57.09 +16:59:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:11.93 +17:42:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:22.29 +16:14:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:25.45 +13:28:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:28.12 +13:50:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:30.86 +14:52:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:32.45 +16:29:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:46.63 +14:47:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:54.56 +14:51:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:55.00 +17:26:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:05.92 +16:19:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:09.03 +17:31:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:10.67 +17:30:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:23.33 +15:36:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:23.67 +14:49:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:31.89 +13:26:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:37.12 +15:28:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:38.99 +15:16:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:39.40 +15:01:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:44.51 +17:21:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:51.37 +15:43:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:59.01 +17:22:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:18.14 +15:12:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:20.08 +10:02:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:21.10 +15:28:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:26.70 +15:00:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:28.12 +15:20:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:31.19 +15:20:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:48.01 +15:57:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:57.12 +17:26:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:58.78 +16:22:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:10.18 +12:55:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:17.34 +11:55:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:19.53 +14:42:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:23.70 +17:13:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:27.53 +14:13:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:31.18 +17:23:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:39.25 +12:47:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:44.01 +14:52:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:47.44 +15:24:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:49.71 +12:47:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:50.81 +14:44:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:07.62 +18:00:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:08.40 +17:22:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:14.15 +13:14:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:21.65 +14:20:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:22.25 +10:07:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:33.77 +14:45:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:35.48 +11:15:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:35.97 +13:49:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:37.19 +16:02:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:42.27 +15:10:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:00.70 +14:58:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:10.86 +14:43:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:16.16 +15:59:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:27.39 +14:45:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:27.96 +14:23:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:32.34 +13:47:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:37.99 +17:53:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:50.94 +17:58:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:53.67 +14:10:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:54.44 +12:55:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:57.83 +15:45:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:19.10 +12:58:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:19.71 +14:31:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:27.35 +16:42:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:28.87 +15:12:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:58.67 +18:09:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:01.32 +18:06:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:02.23 +15:48:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:11.07 +15:50:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:11.51 +12:04:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:24.85 +10:19:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:35.47 +14:21:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:44.87 +14:40:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:50.72 +16:23:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:52.57 +15:42:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:55.26 +14:42:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:00.48 +17:37:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:12.86 +17:18:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:18.07 +14:22:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:21.39 +17:01:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:28.69 +14:20:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:34.84 +14:20:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:42.41 +17:53:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:51.02 +14:40:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:54.39 +11:33:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:02.13 +16:47:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:04.36 +16:47:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:12.08 +12:45:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:32.57 +13:26:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:36.57 +17:40:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:42.37 +15:59:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:47.12 +16:38:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:59.21 +17:10:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:01.74 +13:52:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:16.95 +13:20:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:24.74 +14:14:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:26.34 +17:59:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:35.52 +13:38:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:39.35 +13:04:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:42.81 +17:46:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:46.73 +15:42:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:57.41 +16:50:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:58.44 +14:41:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:23.34 +13:14:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:30.97 +15:43:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:31.34 +14:40:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:40.48 +17:48:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:43.42 +12:44:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:47.10 +17:02:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:53.66 +13:08:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:11.59 +16:05:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:17.55 +14:40:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:30.13 +11:14:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:30.72 +15:36:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:49.20 +16:28:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:49.25 +16:41:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:04.23 +16:36:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:09.40 +15:58:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:33.68 +17:35:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:36.63 +13:37:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:36.83 +14:06:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:46.57 +17:09:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:01.08 +16:39:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:01.11 +16:56:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:02.09 +15:47:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:25.39 +17:42:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:36.79 +17:47:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:56.70 +16:47:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:05.36 +15:18:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:07.91 +16:55:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:16.30 +15:59:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:31.25 +15:16:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:44.20 +17:39:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:51.97 +16:41:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:19.35 +16:19:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:29.58 +15:24:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:27.64 +13:42:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:29.54 +15:00:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:42.38 +16:47:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:46.63 +18:03:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:06.16 +18:09:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:24.25 +14:54:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:37.70 +17:57:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:00.95 +16:03:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:28.25 +17:43:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:47.10 +15:31:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:06.81 +12:37:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:13.58 +13:05:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:15.89 +17:59:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:42.85 +11:12:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:48.45 +13:57:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:09.24 +15:02:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:17.59 +13:56:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:24.91 +16:31:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:09.43 +14:33:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:18.37 +18:02:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:47.79 +16:51:34.7 -- 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)
05:48:08.74 +15:56:46.3 -- not a known variable star
05:48:32.31 +11:28:52.5 -- not a known variable star
05:48:37.32 +15:50:58.7 -- a known variable star
05:48:53.13 +10:13:09.1 -- not a known variable star
05:49:14.22 +14:41:49.9 -- a known variable star
05:49:16.39 +11:26:25.1 -- not a known variable star
05:49:28.19 +11:30:41.1 -- not a known variable star
05:49:29.16 +13:54:40.7 -- not a known variable star
05:49:48.99 +11:48:49.0 -- not a known variable star
05:49:53.50 +12:29:45.4 -- not a known variable star
05:50:03.76 +10:24:30.6 -- a known variable star
05:50:05.21 +10:34:52.9 -- not a known variable star
05:50:07.25 +15:27:57.1 -- not a known variable star
05:50:13.32 +13:10:47.3 -- a known variable star
05:50:15.64 +13:10:20.9 -- not a known variable star
05:50:15.94 +13:54:06.7 -- not a known variable star
05:50:27.70 +15:04:18.3 -- not a known variable star
05:50:50.22 +14:25:30.8 -- not a known variable star
05:51:00.51 +13:29:08.8 -- a known variable star
05:51:05.92 +15:39:54.3 -- not a known variable star
05:51:06.30 +15:03:04.4 -- not a known variable star
05:51:14.90 +14:02:32.7 -- not a known variable star
05:51:19.82 +13:57:03.9 -- not a known variable star
05:51:24.63 +13:40:34.6 -- a known variable star
05:51:31.58 +15:47:51.0 -- not a known variable star
05:51:44.60 +15:34:43.5 -- not a known variable star
05:51:44.66 +14:17:01.2 -- not a known variable star
05:52:03.63 +15:17:57.9 -- not a known variable star
05:52:18.21 +15:51:58.5 -- not a known variable star
05:52:19.39 +15:41:14.0 -- not a known variable star
05:52:22.26 +14:25:29.3 -- not a known variable star
05:52:23.63 +14:54:07.5 -- not a known variable star
05:52:24.06 +13:07:42.1 -- not a known variable star
05:52:33.54 +15:43:51.8 -- a known variable star
05:52:38.40 +15:49:35.6 -- not a known variable star
05:52:46.77 +15:24:02.9 -- not a known variable star
05:52:57.06 +13:18:07.9 -- not a known variable star
05:53:11.70 +14:46:13.7 -- not a known variable star
05:53:13.24 +14:40:26.3 -- not a known variable star
05:53:52.19 +10:13:57.5 -- not a known variable star
05:54:02.77 +14:48:32.4 -- not a known variable star
05:54:03.01 +13:05:40.2 -- not a known variable star
05:54:12.38 +15:02:21.1 -- not a known variable star
05:54:18.55 +15:25:19.1 -- not a known variable star
05:54:30.03 +14:48:43.8 -- not a known variable star
05:54:30.48 +12:57:31.2 -- not a known variable star
05:55:03.80 +15:54:25.8 -- a known variable star
05:55:13.00 +12:41:16.7 -- not a known variable star
05:55:21.77 +15:39:09.2 -- a known variable star
05:55:23.29 +14:46:09.8 -- not a known variable star
05:55:28.40 +12:46:35.7 -- not a known variable star
05:55:30.15 +15:07:43.0 -- not a known variable star
05:55:31.00 +15:11:03.4 -- not a known variable star
05:55:47.19 +14:48:03.3 -- not a known variable star
05:55:50.23 +17:41:16.2 -- not a known variable star
05:55:56.50 +14:38:13.7 -- not a known variable star
05:55:56.82 +17:18:04.4 -- not a known variable star
05:55:57.23 +16:32:15.4 -- a known variable star
05:56:00.70 +11:46:10.3 -- not a known variable star
05:56:00.89 +15:07:20.7 -- not a known variable star
05:56:04.67 +16:54:40.0 -- not a known variable star
05:56:09.13 +17:46:33.2 -- not a known variable star
05:56:16.27 +12:14:41.5 -- not a known variable star
05:56:21.71 +17:58:16.1 -- not a known variable star
05:56:33.13 +15:24:54.7 -- not a known variable star
05:56:34.56 +10:29:34.4 -- not a known variable star
05:56:40.30 +16:06:18.8 -- not a known variable star
05:56:44.03 +17:00:10.6 -- not a known variable star
05:56:47.22 +17:56:00.9 -- not a known variable star
05:56:51.70 +12:21:05.0 -- not a known variable star
05:57:00.08 +17:55:39.2 -- not a known variable star
05:57:00.12 +13:28:56.6 -- not a known variable star
05:57:06.30 +17:40:03.3 -- not a known variable star
05:57:13.85 +17:08:13.1 -- not a known variable star
05:57:13.85 +17:30:31.4 -- not a known variable star
05:57:29.14 +16:25:49.5 -- not a known variable star
05:57:29.25 +10:49:42.8 -- not a known variable star
05:57:29.86 +16:51:07.0 -- not a known variable star
05:57:33.47 +10:55:27.7 -- not a known variable star
05:57:33.70 +15:38:37.6 -- not a known variable star
05:57:35.03 +15:59:00.1 -- not a known variable star
05:57:35.31 +17:58:56.7 -- not a known variable star
05:57:37.01 +16:32:37.8 -- not a known variable star
05:57:42.27 +15:57:13.2 -- a known variable star
05:57:44.30 +13:34:32.9 -- not a known variable star
05:57:54.95 +15:49:12.1 -- not a known variable star
05:57:55.44 +13:34:11.1 -- not a known variable star
05:58:02.29 +16:49:20.9 -- not a known variable star
05:58:07.30 +16:38:48.8 -- not a known variable star
05:58:23.29 +14:59:59.7 -- not a known variable star
05:58:26.36 +15:59:27.8 -- not a known variable star
05:58:27.75 +14:56:55.0 -- not a known variable star
05:58:27.76 +15:59:40.1 -- not a known variable star
05:58:29.54 +15:03:34.6 -- not a known variable star
05:58:30.34 +17:44:47.9 -- not a known variable star
05:58:30.36 +17:12:37.4 -- not a known variable star
05:58:48.36 +13:38:12.1 -- not a known variable star
05:58:48.37 +16:29:35.8 -- not a known variable star
05:58:52.27 +13:37:22.3 -- not a known variable star
05:59:02.80 +14:46:12.3 -- a known variable star
05:59:04.15 +15:40:37.4 -- not a known variable star
05:59:07.20 +15:23:10.3 -- not a known variable star
05:59:11.19 +16:41:15.8 -- not a known variable star
05:59:14.49 +14:14:26.2 -- not a known variable star
05:59:25.67 +15:07:24.7 -- not a known variable star
05:59:32.63 +13:11:26.7 -- not a known variable star
05:59:54.48 +16:54:38.7 -- not a known variable star
05:59:56.19 +11:30:34.1 -- not a known variable star
05:59:57.47 +13:03:23.9 -- not a known variable star
05:59:57.80 +17:18:57.4 -- not a known variable star
06:00:02.61 +11:09:52.3 -- not a known variable star
06:00:12.83 +10:48:38.6 -- not a known variable star
06:00:15.39 +12:08:18.0 -- not a known variable star
06:00:20.50 +15:32:27.3 -- not a known variable star
06:00:36.43 +11:03:23.1 -- not a known variable star
06:00:38.09 +15:37:19.4 -- not a known variable star
06:00:38.27 +15:56:45.7 -- not a known variable star
06:00:51.32 +16:19:51.9 -- not a known variable star
06:00:51.40 +10:59:28.2 -- not a known variable star
06:00:57.41 +16:27:52.0 -- not a known variable star
06:00:57.68 +14:31:57.1 -- not a known variable star
06:01:12.93 +14:02:43.4 -- not a known variable star
06:01:14.33 +14:32:07.9 -- not a known variable star
06:01:19.48 +15:34:36.6 -- a known variable star
06:01:20.72 +17:26:15.5 -- not a known variable star
06:01:21.00 +12:23:32.8 -- not a known variable star
06:01:23.34 +13:54:28.3 -- not a known variable star
06:01:33.03 +12:58:52.5 -- not a known variable star
06:01:37.27 +15:19:51.9 -- a known variable star
06:01:37.68 +14:43:11.4 -- not a known variable star
06:01:42.11 +16:14:30.9 -- not a known variable star
06:01:45.31 +11:15:08.8 -- not a known variable star
06:02:07.56 +15:11:23.2 -- not a known variable star
06:02:07.79 +16:23:46.6 -- not a known variable star
06:02:09.43 +13:56:17.9 -- not a known variable star
06:02:09.67 +12:11:04.5 -- not a known variable star
06:02:12.38 +12:06:06.2 -- not a known variable star
06:02:21.36 +16:12:34.2 -- not a known variable star
06:02:23.83 +16:35:57.0 -- not a known variable star
06:02:38.41 +14:07:58.5 -- not a known variable star
06:03:20.61 +10:39:27.7 -- not a known variable star
06:03:24.37 +14:38:53.9 -- not a known variable star
06:03:45.62 +14:20:46.8 -- not a known variable star
06:03:52.31 +14:59:06.2 -- a known variable star
06:03:54.47 +12:44:04.2 -- a known variable star
06:04:09.22 +15:25:54.2 -- not a known variable star
06:04:11.35 +12:35:21.9 -- a known variable star
06:04:18.72 +12:32:52.4 -- not a known variable star
06:04:26.30 +18:02:07.7 -- not a known variable star
06:04:28.03 +16:29:14.2 -- not a known variable star
06:04:31.59 +15:26:09.2 -- a known variable star
06:05:20.88 +15:10:13.7 -- a known variable star
06:05:37.22 +17:10:44.5 -- not a known variable star
06:05:46.85 +10:58:59.2 -- not a known variable star
06:05:57.84 +11:37:35.4 -- not a known variable star
06:06:00.97 +16:53:36.4 -- not a known variable star
06:06:05.15 +13:21:02.3 -- not a known variable star
06:06:13.09 +16:19:25.9 -- not a known variable star
06:06:25.19 +16:38:04.6 -- not a known variable star
06:06:40.77 +15:11:24.5 -- not a known variable star
06:06:48.48 +16:40:37.7 -- not a known variable star
06:06:48.49 +16:49:38.2 -- not a known variable star
06:06:57.44 +18:07:52.5 -- not a known variable star
06:06:58.48 +14:36:07.6 -- not a known variable star
06:07:01.07 +10:58:45.7 -- a known variable star
06:07:05.39 +10:57:47.3 -- not a known variable star
06:07:08.68 +12:32:31.1 -- not a known variable star
06:07:09.40 +16:42:46.9 -- not a known variable star
06:08:08.26 +14:27:05.4 -- not a known variable star
06:08:14.29 +13:57:07.0 -- a known variable star
06:08:22.48 +11:49:59.2 -- not a known variable star
06:08:27.07 +16:23:02.2 -- not a known variable star
06:08:32.34 +12:55:13.0 -- not a known variable star
06:08:55.81 +17:07:39.8 -- not a known variable star
06:09:12.73 +15:40:26.2 -- a known variable star
06:09:30.91 +13:08:59.7 -- not a known variable star
06:09:52.24 +11:19:55.9 -- a known variable star
06:09:52.59 +14:42:45.0 -- not a known variable star
06:09:55.61 +14:26:05.8 -- not a known variable star
06:09:57.09 +16:59:12.5 -- not a known variable star
06:10:11.93 +17:42:34.7 -- not a known variable star
06:10:22.29 +16:14:32.2 -- not a known variable star
06:10:25.45 +13:28:04.0 -- not a known variable star
06:10:28.12 +13:50:01.6 -- a known variable star
06:10:30.86 +14:52:41.5 -- not a known variable star
06:10:32.45 +16:29:31.2 -- not a known variable star
06:10:46.63 +14:47:20.1 -- not a known variable star
06:10:54.56 +14:51:53.8 -- not a known variable star
06:10:55.00 +17:26:53.0 -- not a known variable star
06:11:05.92 +16:19:10.0 -- not a known variable star
06:11:09.03 +17:31:03.4 -- not a known variable star
06:11:10.67 +17:30:32.5 -- not a known variable star
06:11:23.33 +15:36:18.7 -- not a known variable star
06:11:23.67 +14:49:43.8 -- not a known variable star
06:11:31.89 +13:26:07.7 -- not a known variable star
06:11:37.12 +15:28:25.8 -- not a known variable star
06:11:38.99 +15:16:52.1 -- not a known variable star
06:11:39.40 +15:01:29.1 -- not a known variable star
06:11:44.51 +17:21:10.0 -- not a known variable star
06:11:51.37 +15:43:45.7 -- not a known variable star
06:11:59.01 +17:22:43.5 -- not a known variable star
06:12:18.14 +15:12:21.6 -- not a known variable star
06:12:20.08 +10:02:02.9 -- not a known variable star
06:12:21.10 +15:28:31.8 -- a known variable star
06:12:26.70 +15:00:24.6 -- not a known variable star
06:12:28.12 +15:20:04.0 -- not a known variable star
06:12:31.19 +15:20:14.8 -- not a known variable star
06:12:48.01 +15:57:44.1 -- not a known variable star
06:12:57.12 +17:26:20.8 -- a known variable star
06:12:58.78 +16:22:06.4 -- not a known variable star
06:13:10.18 +12:55:19.3 -- not a known variable star
06:13:17.34 +11:55:02.2 -- not a known variable star
06:13:19.53 +14:42:59.0 -- not a known variable star
06:13:23.70 +17:13:26.2 -- not a known variable star
06:13:27.53 +14:13:51.9 -- a known variable star
06:13:31.18 +17:23:07.5 -- a known variable star
06:13:39.25 +12:47:36.1 -- not a known variable star
06:13:44.01 +14:52:17.4 -- not a known variable star
06:13:47.44 +15:24:03.1 -- not a known variable star
06:13:49.71 +12:47:05.9 -- not a known variable star
06:13:50.81 +14:44:31.5 -- not a known variable star
06:14:07.62 +18:00:35.7 -- not a known variable star
06:14:08.40 +17:22:59.2 -- not a known variable star
06:14:14.15 +13:14:59.7 -- a known variable star
06:14:21.65 +14:20:39.0 -- not a known variable star
06:14:22.25 +10:07:40.1 -- not a known variable star
06:14:33.77 +14:45:32.8 -- not a known variable star
06:14:35.48 +11:15:30.7 -- a known variable star
06:14:35.97 +13:49:52.3 -- not a known variable star
06:14:37.19 +16:02:30.0 -- not a known variable star
06:14:42.27 +15:10:59.3 -- not a known variable star
06:15:00.70 +14:58:53.8 -- not a known variable star
06:15:10.86 +14:43:50.2 -- not a known variable star
06:15:16.16 +15:59:57.2 -- not a known variable star
06:15:27.39 +14:45:49.8 -- a known variable star
06:15:27.96 +14:23:53.8 -- not a known variable star
06:15:32.34 +13:47:36.2 -- not a known variable star
06:15:37.99 +17:53:12.9 -- not a known variable star
06:15:50.94 +17:58:52.8 -- not a known variable star
06:15:53.67 +14:10:16.5 -- not a known variable star
06:15:54.44 +12:55:37.6 -- not a known variable star
06:15:57.83 +15:45:45.1 -- a known variable star
06:16:19.10 +12:58:42.3 -- not a known variable star
06:16:19.71 +14:31:17.4 -- not a known variable star
06:16:27.35 +16:42:37.0 -- a known variable star
06:16:28.87 +15:12:39.8 -- not a known variable star
06:16:58.67 +18:09:12.6 -- not a known variable star
06:17:01.32 +18:06:38.1 -- not a known variable star
06:17:02.23 +15:48:27.1 -- a known variable star
06:17:11.07 +15:50:13.9 -- a known variable star
06:17:11.51 +12:04:06.2 -- a known variable star
06:17:24.85 +10:19:34.6 -- a known variable star
06:17:35.47 +14:21:38.3 -- not a known variable star
06:17:44.87 +14:40:48.6 -- a known variable star
06:17:50.72 +16:23:57.8 -- not a known variable star
06:17:52.57 +15:42:08.5 -- not a known variable star
06:17:55.26 +14:42:53.9 -- a known variable star
06:18:00.48 +17:37:01.4 -- not a known variable star
06:18:12.86 +17:18:43.0 -- not a known variable star
06:18:18.07 +14:22:18.5 -- not a known variable star
06:18:21.39 +17:01:39.7 -- not a known variable star
06:18:28.69 +14:20:27.4 -- not a known variable star
06:18:34.84 +14:20:07.9 -- not a known variable star
06:18:42.41 +17:53:58.5 -- a known variable star
06:18:51.02 +14:40:00.2 -- a known variable star
06:18:54.39 +11:33:58.2 -- not a known variable star
06:19:02.13 +16:47:08.0 -- not a known variable star
06:19:04.36 +16:47:19.7 -- not a known variable star
06:19:12.08 +12:45:05.6 -- a known variable star
06:19:32.57 +13:26:12.2 -- not a known variable star
06:19:36.57 +17:40:29.3 -- not a known variable star
06:19:42.37 +15:59:26.5 -- not a known variable star
06:19:47.12 +16:38:52.2 -- not a known variable star
06:19:59.21 +17:10:05.3 -- not a known variable star
06:20:01.74 +13:52:51.3 -- not a known variable star
06:20:16.95 +13:20:08.4 -- not a known variable star
06:20:24.74 +14:14:42.3 -- not a known variable star
06:20:26.34 +17:59:04.0 -- not a known variable star
06:20:35.52 +13:38:05.2 -- not a known variable star
06:20:39.35 +13:04:20.9 -- not a known variable star
06:20:42.81 +17:46:45.8 -- not a known variable star
06:20:46.73 +15:42:08.3 -- not a known variable star
06:20:57.41 +16:50:14.0 -- not a known variable star
06:20:58.44 +14:41:23.0 -- a known variable star
06:21:23.34 +13:14:45.8 -- not a known variable star
06:21:30.97 +15:43:18.3 -- not a known variable star
06:21:31.34 +14:40:25.4 -- not a known variable star
06:21:40.48 +17:48:04.2 -- not a known variable star
06:21:43.42 +12:44:20.6 -- not a known variable star
06:21:47.10 +17:02:50.5 -- not a known variable star
06:21:53.66 +13:08:31.1 -- not a known variable star
06:22:11.59 +16:05:21.9 -- not a known variable star
06:22:17.55 +14:40:26.2 -- not a known variable star
06:23:30.13 +11:14:21.5 -- a known variable star
06:23:30.72 +15:36:13.9 -- not a known variable star
06:23:49.20 +16:28:13.7 -- not a known variable star
06:24:49.25 +16:41:34.4 -- not a known variable star
06:25:04.23 +16:36:40.2 -- not a known variable star
06:25:09.40 +15:58:53.2 -- not a known variable star
06:25:33.68 +17:35:13.7 -- not a known variable star
06:25:36.63 +13:37:50.3 -- not a known variable star
06:25:36.83 +14:06:33.7 -- not a known variable star
06:25:46.57 +17:09:24.5 -- not a known variable star
06:26:01.08 +16:39:51.4 -- a known variable star
06:26:01.11 +16:56:24.1 -- not a known variable star
06:26:02.09 +15:47:59.3 -- not a known variable star
06:26:25.39 +17:42:20.4 -- a known variable star
06:26:36.79 +17:47:21.8 -- not a known variable star
06:26:56.70 +16:47:33.6 -- not a known variable star
06:27:05.36 +15:18:40.6 -- not a known variable star
06:27:07.91 +16:55:02.4 -- not a known variable star
06:27:16.30 +15:59:50.2 -- not a known variable star
06:27:31.25 +15:16:12.9 -- not a known variable star
06:27:44.20 +17:39:44.9 -- not a known variable star
06:27:51.97 +16:41:06.2 -- a known variable star
06:28:19.35 +16:19:07.2 -- not a known variable star
06:28:29.58 +15:24:33.8 -- not a known variable star
06:30:27.64 +13:42:19.9 -- not a known variable star
06:31:29.54 +15:00:32.2 -- not a known variable star
06:31:42.38 +16:47:43.8 -- a known variable star
06:31:46.63 +18:03:22.1 -- not a known variable star
06:32:06.16 +18:09:36.7 -- not a known variable star
06:32:24.25 +14:54:07.7 -- not a known variable star
06:32:37.70 +17:57:41.0 -- not a known variable star
06:33:00.95 +16:03:44.3 -- not a known variable star
06:34:28.25 +17:43:05.2 -- not a known variable star
06:34:47.10 +15:31:02.4 -- not a known variable star
06:35:06.81 +12:37:59.2 -- a known variable star
06:36:13.58 +13:05:53.3 -- not a known variable star
06:36:15.89 +17:59:27.2 -- not a known variable star
06:36:42.85 +11:12:37.7 -- not a known variable star
06:37:48.45 +13:57:17.5 -- not a known variable star
06:38:09.24 +15:02:40.6 -- not a known variable star
06:38:17.59 +13:56:19.0 -- not a known variable star
06:38:24.91 +16:31:42.9 -- a known variable star
06:40:09.43 +14:33:37.8 -- not a known variable star
06:41:18.37 +18:02:06.5 -- not a known variable star
06:41:47.79 +16:51:34.7 -- a known variable star
Found 287 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
338 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 338 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461128.62198786 -observatory 500
22:51:37.34 -08:08:39.1 Mercury (0.5mag)
01:43:47.88 +10:08:29.0 Venus (-3.9mag)
23:26:44.07 -04:44:02.1 Mars (1.2mag)
07:06:19.29 +22:55:56.9 Jupiter (-2.2mag)
00:21:04.34 -00:02:14.1 Saturn (0.9mag)
03:44:15.14 +19:36:15.9 Uranus (5.8mag)
00:08:25.16 -00:30:45.8 Neptune (7.8mag)
20:32:40.71 -22:52:54.9 Pluto (14.5mag)
09:33:19.98 +16:13:15.8 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Mar 28 22:00 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461128.62198786:
07:06:12.55 +22:56:11.3 Io (5.7mag)
07:06:19.69 +22:55:59.3 Europa (5.8mag)
07:06:00.62 +22:56:36.2 Ganymede (5.2mag)
07:06:52.22 +22:54:59.6 Callisto (6.5mag)
07:10:14.94 +22:52:52.7 Himalia (15.2mag)
07:06:16.97 +22:56:03.5 Thebe (16.1mag)
07:10:00.74 +23:19:21.8 Elara (17.2mag)
07:03:59.45 +23:45:20.0 Pasiphae (17.3mag)
07:14:59.57 +22:51:46.1 Carme (18.4mag)
00:21:12.39 -00:01:59.8 Titan (8.8mag)
00:21:03.42 -00:02:09.1 Rhea (10.1mag)
00:21:22.49 -00:00:04.6 Iapetus (11.5mag)
00:20:59.39 -00:01:48.2 Hyperion (14.8mag)
00:22:53.85 +00:08:20.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 28 22:00 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461128.62198786:
13:53:03.05 +00:00:39.8 JWST
16:24:03.62 +48:30:34.6 Chandra
07:50:19.27 -26:47:15.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 28 22:00 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461128.62198786 -observatory 500
18:41:49.15 -27:50:01.1 14.0mag P/2010 H2 (Vales)
04:55:17.53 -70:34:41.6 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:26.63 +31:20:02.1 17.1mag C/2017 K2 (PANSTARRS)
17:30:37.79 +08:23:18.7 17.6mag C/2021 G2 (ATLAS)
23:04:36.56 +28:37:25.8 17.0mag C/2022 E2 (ATLAS)
04:09:05.09 +25:31:49.2 15.8mag C/2022 N2 (PANSTARRS)
09:01:28.46 +31:43:26.6 16.1mag C/2022 QE78 (ATLAS)
08:29:46.53 -02:10:49.8 17.2mag C/2022 R6 (PANSTARRS)
18:56:22.30 +16:59:37.6 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:14.21 -11:45:42.1 17.6mag P/2023 B1 (PANSTARRS)
09:18:11.08 -14:53:51.7 17.5mag C/2023 F3 (ATLAS)
21:33:14.71 +62:00:02.5 17.4mag C/2023 H5 (Lemmon)
19:30:30.40 -03:33:08.3 14.4mag C/2023 R1 (PANSTARRS)
21:41:43.80 +83:40:00.0 17.8mag C/2023 X2 (Lemmon)
06:13:51.96 +63:40:36.7 16.9mag C/2024 A1 (ATLAS)
04:30:24.58 +10:30:08.1 9.8mag C/2024 E1 (Wierzchos)
16:29:04.39 +03:27:37.8 17.4mag C/2024 G6 (ATLAS)
20:14:06.63 +10:40:27.1 14.8mag C/2024 J3 (ATLAS)
03:11:03.66 -25:15:20.2 16.4mag C/2024 T5 (ATLAS)
05:02:44.81 +50:07:02.6 17.6mag C/2025 J1 (Borisov)
14:48:58.63 +28:10:49.1 14.5mag C/2025 L1 (ATLAS)
02:59:03.39 -23:38:14.9 17.7mag C/2025 Q3 (ATLAS)
22:39:46.36 +19:32:45.4 11.4mag C/2025 R3 (PANSTARRS)
13:01:49.77 +01:51:21.7 17.6mag C/2025 Y1 (ATLAS)
01:44:20.66 -00:58:08.5 11.6mag C/2026 A1 (MAPS)
23:05:36.89 +33:18:44.9 14.0mag C/2026 B2 (Sun-Gao)
18:07:59.38 -10:33:58.9 12.9mag 10P/Tempel
15:21:15.29 +04:40:57.7 12.5mag 24P/Schaumasse
11:08:42.39 -02:10:01.6 15.7mag 29P/Schwassmann-Wachmann
17:51:09.51 -10:19:25.7 17.5mag 40P/Vaisala
10:41:24.61 -05:44:08.3 16.6mag 43P/Wolf-Harrington
01:21:14.07 +14:22:30.7 17.1mag 47P/Ashbrook-Jackson
06:40:16.22 +40:43:37.6 17.1mag 63P/Wild
23:05:26.99 -13:40:56.3 15.7mag 65P/Gunn
03:17:40.68 +14:37:32.2 15.9mag 76P/West-Kohoutek-Ikemura
00:26:42.99 +04:40:17.7 14.5mag 78P/Gehrels
22:06:16.57 -14:33:51.9 14.5mag 88P/Howell
01:21:39.01 +15:37:30.2 15.2mag 93P/Lovas
04:23:17.04 +31:13:14.0 16.4mag 123P/West-Hartley
08:11:32.69 +46:35:59.3 16.2mag 124P/Mrkos
02:06:10.30 +12:18:57.6 16.4mag 128P/Shoemaker-Holt
02:12:51.08 +12:10:13.8 17.4mag 131P/Mueller
23:56:54.98 +06:22:50.7 12.0mag 141P/Machholz
00:07:11.08 -01:42:40.3 12.1mag 141P-A/Machholz
23:02:43.37 -04:49:11.9 15.1mag 141P-D/Machholz
00:12:50.97 -10:20:15.5 15.3mag 162P/SidingSpring
10:34:23.82 +31:52:53.4 17.7mag 164P/Christensen
06:03:53.24 +24:40:04.4 17.7mag 198P/ODAS
15:21:53.75 -02:15:29.9 17.1mag 210P/Christensen
20:41:41.31 -15:44:08.6 17.3mag 218P/LINEAR
17:06:58.09 -15:55:26.1 16.2mag 235P/LINEAR
04:57:13.38 +33:00:04.9 16.5mag 240P/NEAT
07:31:35.47 -07:17:40.8 17.6mag 242P/Spahr
15:47:42.71 +05:42:44.0 17.6mag 391P/Kowalski
07:29:03.45 +21:13:39.5 17.6mag 450P/LONEOS
05:11:06.40 +46:06:04.8 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Mar 28 22:00 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
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
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
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
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
18:38:35.79 -79:28:57.30 ASASSN-26bb 2026-02-24.37 16.2
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
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
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
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
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
-rw-r--r-- 1 apache apache 5.8K Mar 28 22:00 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 28 22:00 tocp_transients_list.txt