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_223337_TTUQ2b1x1_704_qspcU5Q4
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,2461128.6232,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.1232 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:44.94 +11:17:01.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.37 06:17:32.29 +16:47:23.0
194.18280 0.35198 galactic Ori Second-epoch detections are separated by 2.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:17:32.29 +16:47:23.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 17 32.29 +16 47 23.0 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,2461128.6232,14.37,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:32.29 +16:47:23.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 02 38.33 +14 07 59.3 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,2461128.6232,14.37,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:38.33 +14:07:59.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 16 41.50 +14 25 10.4 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,2461128.6232,14.20,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:41.50 +14:25:10.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 15 49.41 +13 13 07.8 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,2461128.6232,14.37,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:49.41 +13:13:07.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 19 01.55 +14 21 47.0 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,2461128.6232,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:01.55 +14:21:47.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.26 05:54:48.72 +13:47:50.8
194.13240 -5.89103 galactic Ori Second-epoch detections are separated by 5.5" and 2.4 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 | 05:54:48.72 +13:47:50.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 54 48.72 +13 47 50.8 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
target,2461128.6232,14.26,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:48.72 +13:47:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.21 06:25:19.99 +15:08:17.2
196.52186 1.22823 galactic Ori Second-epoch detections are separated by 2.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.3292+15.1402 | 06:25:19.99 +15:08:17.2 (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 29.1232* 06 25 19.99 +15 08 17.2 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 J096.3292+15.1402,2461128.6232,14.21,0.05,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 J096.3292+15.1402 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:19.99 +15:08:17.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.33 06:16:49.33 +14:56:25.0
195.72874 -0.67771 galactic Ori Second-epoch detections are separated by 1.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J094.2111+14.9344 | 06:16:49.33 +14:56:25.0 (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 29.1232* 06 16 49.33 +14 56 25.0 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 J094.2111+14.9344,2461128.6232,14.33,0.05,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 J094.2111+14.9344 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:49.33 +14:56:25.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 12 29.71 +12 51 00.4 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
Gaia DR3 3343992031213748608,2461128.6232,14.28,0.05,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 3343992031213748608 20260329.1232 14.28CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:29.71 +12:51:00.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.39 06:08:08.32 +14:27:06.1
195.15037 -2.75470 galactic Ori Second-epoch detections are separated by 3.9" and 2.9 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 | 06:08:08.32 +14:27:06.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 08 08.32 +14 27 06.1 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
target,2461128.6232,14.39,0.05,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
target 20260329.1232 14.39CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:08.32 +14:27:06.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 20 10.22 +12 07 10.0 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 3331739520307963136,2461128.6232,14.14,0.05,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
Gaia DR3 3331739520307963136 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:10.22 +12:07:10.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.51 06:04:08.81 +11:12:57.6
197.51547 -5.17339 galactic Ori Second-epoch detections are separated by 5.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:04:08.81 +11:12:57.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 04 08.81 +11 12 57.6 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,2461128.6232,14.51,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:08.81 +11:12:57.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.15 06:03:03.62 +13:25:03.3
195.45577 -4.33419 galactic Ori Second-epoch detections are separated by 4.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:03:03.62 +13:25:03.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 03 03.62 +13 25 03.3 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,2461128.6232,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:03.62 +13:25:03.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 07 50.05 +12 50 04.1 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
target,2461128.6232,14.44,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:50.05 +12:50:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.46 05:57:25.12 +15:34:07.5
192.90362 -4.46368 galactic Ori Second-epoch detections are separated by 2.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.3459+15.5742 | 05:57:25.12 +15:34:07.5 (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 29.1232* 05 57 25.12 +15 34 07.5 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 J089.3459+15.5742,2461128.6232,14.46,0.05,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 J089.3459+15.5742 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:25.12 +15:34:07.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.36 05:58:51.50 +15:39:36.4
192.99638 -4.11735 galactic Ori Second-epoch detections are separated by 4.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:58:51.50 +15:39:36.4 (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 29.1232* 05 58 51.50 +15 39 36.4 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,2461128.6232,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:51.50 +15:39:36.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.10 06:28:32.96 +15:25:10.6
196.63343 2.04579 galactic Gem Second-epoch detections are separated by 6.0" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.1355+15.4140 | 06:28:32.96 +15:25:10.6 (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 J097.1355+15.4140,2461128.6232,14.10,0.05,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 J097.1355+15.4140 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:32.96 +15:25:10.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.44 05:50:29.23 +15:16:05.2
192.32550 -6.06041 galactic Tau Second-epoch detections are separated by 1.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J087.6256+15.2594 | 05:50:29.23 +15:16:05.2 (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 29.1232* 05 50 29.23 +15 16 05.2 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 J087.6256+15.2594,2461128.6232,14.44,0.05,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
ATO J087.6256+15.2594 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:29.23 +15:16:05.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.28 05:51:58.05 +15:48:26.5
192.03785 -5.48074 galactic Tau Second-epoch detections are separated by 3.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:51:58.05 +15:48:26.5 (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 29.1232* 05 51 58.05 +15 48 26.5 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,2461128.6232,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 14.28CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:58.05 +15:48:26.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 55 21.81 +15 39 09.6 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
Gaia DR3 3348796553430528512,2461128.6232,14.36,0.05,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
Gaia DR3 3348796553430528512 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:21.81 +15:39:09.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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,2461128.6232,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:29.76 +16:46:34.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.08 06:21:43.51 +12:44:21.3
198.23105 -0.66908 galactic Ori Second-epoch detections are separated by 2.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 21 43.51 +12 44 21.3 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
Gaia DR3 3332188460353765376,2461128.6232,14.08,0.05,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 3332188460353765376 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:43.51 +12:44:21.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.18 06:08:07.79 +15:55:02.4
193.86588 -2.04680 galactic Ori Second-epoch detections are separated by 2.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.0336+15.9150 | 06:08:07.79 +15:55:02.4 (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 29.1232* 06 08 07.79 +15 55 02.4 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
ATO J092.0336+15.9150,2461128.6232,14.18,0.05,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
ATO J092.0336+15.9150 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:07.79 +15:55:02.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.12 06:07:08.77 +12:32:29.9
196.70815 -3.88963 galactic Ori Second-epoch detections are separated by 3.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 07 08.77 +12 32 29.9 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
Gaia DR3 3342698692005715072,2461128.6232,14.12,0.05,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
Gaia DR3 3342698692005715072 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:08.77 +12:32:29.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.99 05:51:07.57 +10:13:07.3
196.81264 -8.45013 galactic Ori Second-epoch detections are separated by 2.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3336652481859874432 | 05:51:07.76 +10:13:24.2 (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 29.1232* 05 51 07.57 +10 13 07.3 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 3336652481859874432,2461128.6232,13.99,0.05,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 3336652481859874432 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:07.57 +10:13:07.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.12 06:20:58.24 +16:02:33.0
195.23039 0.72422 galactic Ori Second-epoch detections are separated by 3.5" and 2.9 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 J095.2466+16.0299 | 06:20:58.26 +16:02:03.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B6 (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 29.1232* 06 20 58.24 +16 02 33.0 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 J095.2466+16.0299,2461128.6232,14.12,0.05,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 J095.2466+16.0299 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:58.24 +16:02:33.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.38 05:56:05.78 +17:53:51.3
190.72153 -3.57731 galactic Ori Second-epoch detections are separated by 4.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:56:05.78 +17:53:51.3 (user input) | T | P | (position from user input) SpType: K5 (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 29.1232* 05 56 05.78 +17 53 51.3 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,2461128.6232,14.38,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:05.78 +17:53:51.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.19 05:57:50.52 +15:53:33.9
192.67228 -4.21440 galactic Ori Second-epoch detections are separated by 3.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3348822220155245696 | 05:57:52.14 +15:53:27.8 (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 29.1232* 05 57 50.52 +15 53 33.9 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 3348822220155245696,2461128.6232,14.19,0.05,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 3348822220155245696 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:50.52 +15:53:33.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.09 06:35:48.68 +18:02:11.9
195.10319 4.79138 galactic Gem Second-epoch detections are separated by 2.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:35:48.68 +18:02:11.9 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6232,14.09,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:48.68 +18:02:11.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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,2461128.6232,14.04,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:19.20 +14:30:00.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.96 06:07:05.41 +10:57:47.1
198.08795 -4.66343 galactic Ori Second-epoch detections are separated by 3.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 07 05.41 +10 57 47.1 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
Gaia DR3 3330233837919819008,2461128.6232,13.96,0.05,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 3330233837919819008 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:05.41 +10:57:47.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.19 05:52:23.96 +13:19:35.4
194.24919 -6.63408 galactic Tau Second-epoch detections are separated by 5.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:52:23.96 +13:19:35.4 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.097 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 52 23.96 +13 19 35.4 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
target,2461128.6232,14.19,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:23.96 +13:19:35.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.09 06:13:51.21 +16:29:05.2
194.03037 -0.56929 galactic Ori Second-epoch detections are separated by 1.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3370105157495668992 | 06:13:49.55 +16:29:08.4 (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 29.1232* 06 13 51.21 +16 29 05.2 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 3370105157495668992,2461128.6232,14.09,0.05,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
Gaia DR3 3370105157495668992 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:51.21 +16:29:05.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 00 30.08 +09 53 10.7 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,2461128.6232,13.98,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:30.08 +09:53:10.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 18 53.63 +17 20 32.0 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
target,2461128.6232,13.96,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:53.63 +17:20:32.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.92 06:41:08.40 +16:06:36.5
197.40584 5.05557 galactic Gem Second-epoch detections are separated by 2.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:41:08.40 +16:06:36.5 (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,2461128.6232,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:08.40 +16:06:36.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.03 05:53:16.81 +14:42:25.5
193.15381 -5.75897 galactic Ori Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3347181744506913280 | 05:53:16.42 +14:43:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 53 16.81 +14 42 25.5 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 3347181744506913280,2461128.6232,14.03,0.05,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 3347181744506913280 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:16.81 +14:42:25.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 10 22.30 +16 14 32.0 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,2461128.6232,14.08,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:22.30 +16:14:32.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 21 24.15 +14 10 53.8 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
target,2461128.6232,14.14,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:24.15 +14:10:53.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.98 05:57:35.34 +17:58:56.2
190.82562 -3.22743 galactic Ori Second-epoch detections are separated by 0.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:57:35.34 +17:58:56.2 (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 29.1232* 05 57 35.34 +17 58 56.2 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,2461128.6232,13.98,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:35.34 +17:58:56.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.87 06:20:25.32 +17:59:14.9
193.45247 1.52447 galactic Gem Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.1052+17.9857 | 06:20:25.32 +17:59:14.9 (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+17.9857,2461128.6232,13.87,0.05,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 J095.1052+17.9857 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:25.32 +17:59:14.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.95 06:40:42.95 +17:09:24.7
196.42144 5.43637 galactic Gem Second-epoch detections are separated by 3.5" and 2.9 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 J100.1836+17.1611 | 06:40:42.95 +17:09:24.7 (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 J100.1836+17.1611,2461128.6232,13.95,0.05,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 J100.1836+17.1611 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:42.95 +17:09:24.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.89 06:03:24.40 +14:38:53.8
194.42051 -3.65957 galactic Ori Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 03 24.40 +14 38 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 3345438846778089728,2461128.6232,13.89,0.05,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 3345438846778089728 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:24.40 +14:38:53.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 20 41.97 +17 05 20.2 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,2461128.6232,14.08,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:41.97 +17:05:20.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.05 06:11:44.47 +17:21:10.7
193.02618 -0.59607 galactic Ori Second-epoch detections are separated by 3.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.9294+17.3499 | 06:11:44.47 +17:21:10.7 (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 29.1232* 06 11 44.47 +17 21 10.7 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
ATO J092.9294+17.3499,2461128.6232,14.05,0.05,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
ATO J092.9294+17.3499 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:44.47 +17:21:10.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.04 05:57:38.21 +16:48:12.8
191.85543 -3.80451 galactic Ori Second-epoch detections are separated by 3.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.4097+16.8092 | 05:57:38.21 +16:48:12.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (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 29.1232* 05 57 38.21 +16 48 12.8 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
ATO J089.4097+16.8092,2461128.6232,14.04,0.05,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 J089.4097+16.8092 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:38.21 +16:48:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 55 49.49 +17 04 43.7 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 3349791577089566848,2461128.6232,14.19,0.05,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 3349791577089566848 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:49.49 +17:04:43.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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,2461128.6232,13.97,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:09.52 +14:11:10.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.06 06:00:38.06 +15:37:20.1
193.24107 -3.76428 galactic Ori Second-epoch detections are separated by 2.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 00 38.06 +15 37 20.1 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 3348655502404916480,2461128.6232,14.06,0.05,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
Gaia DR3 3348655502404916480 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:38.06 +15:37:20.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.13 06:20:06.66 +15:51:59.5
195.28820 0.45903 galactic Ori Second-epoch detections are separated by 5.1" and 2.5 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 J095.0233+15.8661 | 06:20:06.66 +15:51:59.5 (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 29.1232* 06 20 06.66 +15 51 59.5 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
ATO J095.0233+15.8661,2461128.6232,14.13,0.05,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
ATO J095.0233+15.8661 20260329.1232 14.13CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:06.66 +15:51:59.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.19 06:15:50.93 +17:58:53.9
192.94253 0.56395 galactic Ori Second-epoch detections are separated by 2.7" and 2.9 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 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 29.1232* 06 15 50.93 +17 58 53.9 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 3373374241785762944,2461128.6232,14.19,0.05,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 3373374241785762944 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:50.93 +17:58:53.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.93 06:21:19.04 +12:51:49.2
198.07448 -0.69830 galactic Ori Second-epoch detections are separated by 2.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.3293+12.8619 | 06:21:19.04 +12:51:49.2 (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 29.1232* 06 21 19.04 +12 51 49.2 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 J095.3293+12.8619,2461128.6232,13.93,0.05,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 J095.3293+12.8619 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:19.04 +12:51:49.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.94 06:28:49.44 +15:22:57.9
196.69681 2.08737 galactic Gem Second-epoch detections are separated by 1.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.2080+15.3759 | 06:28:49.44 +15:22:57.9 (user input) | CBF (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 J097.2080+15.3759,2461128.6232,13.94,0.05,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 J097.2080+15.3759 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:49.44 +15:22:57.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.79 06:25:36.63 +13:37:49.9
197.88669 0.58399 galactic Gem Second-epoch detections are separated by 3.6" and 2.9 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 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 3332374174738954752,2461128.6232,13.79,0.05,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 3332374174738954752 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:36.63 +13:37:49.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 01 20.73 +13 05 22.2 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,2461128.6232,13.86,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:20.73 +13:05:22.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 13 39.34 +15 30 56.7 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
target,2461128.6232,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:39.34 +15:30:56.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 06 13.05 +16 19 25.1 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,2461128.6232,14.02,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:13.05 +16:19:25.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 57 00.14 +13 28 56.4 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,2461128.6232,13.94,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:00.14 +13:28:56.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 02 12.33 +12 06 05.4 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,2461128.6232,13.88,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:12.33 +12:06:05.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 55 30.14 +15 07 44.4 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,2461128.6232,13.99,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:30.14 +15:07:44.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.96 06:15:20.07 +14:59:21.8
195.51453 -0.97035 galactic Ori Second-epoch detections are separated by 2.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J093.8291+15.0085 | 06:15:19.79 +14:59:55.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0: 1959ApJS....4...23M LF 8 +15 132
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 15 20.07 +14 59 21.8 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
ATO J093.8291+15.0085,2461128.6232,13.96,0.05,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
ATO J093.8291+15.0085 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:20.07 +14:59:21.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 53 57.36 +12 16 41.1 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 3343239106267868928,2461128.6232,13.93,0.05,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
Gaia DR3 3343239106267868928 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:57.36 +12:16:41.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 50 05.30 +10 34 52.5 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
target,2461128.6232,13.85,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:05.30 +10:34:52.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.90 06:02:09.71 +12:11:04.8
196.42835 -5.12703 galactic Ori Second-epoch detections are separated by 4.1" and 2.9 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 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 29.1232* 06 02 09.71 +12 11 04.8 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 3342638493743157888,2461128.6232,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3342638493743157888 20260329.1232 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:09.71 +12:11:04.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.81 06:27:07.95 +16:55:01.9
195.14773 2.43894 galactic Gem Second-epoch detections are separated by 3.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 3369585530874840448,2461128.6232,13.81,0.05,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 3369585530874840448 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:07.95 +16:55:01.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 58 18.72 +18 08 55.4 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 3350451765106102400,2461128.6232,14.01,0.05,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 3350451765106102400 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:18.72 +18:08:55.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 53 22.72 +12 06 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
target,2461128.6232,13.78,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:22.72 +12:06:18.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.76 05:57:16.62 +12:53:47.2
195.21777 -5.81658 galactic Ori Second-epoch detections are separated by 2.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.3304+12.8947 | 05:57:16.62 +12:53:47.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 57 16.62 +12 53 47.2 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 J089.3304+12.8947,2461128.6232,13.76,0.05,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
ATO J089.3304+12.8947 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:16.62 +12:53:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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,2461128.6232,13.85,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:46.12 +17:46:19.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 10 32.47 +16 29 30.3 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
target,2461128.6232,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:32.47 +16:29:30.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.71 05:59:16.87 +12:05:09.6
196.16889 -5.78941 galactic Ori Second-epoch detections are separated by 2.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.8160+12.0897 | 05:59:15.46 +12:05:12.1 (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 29.1232* 05 59 16.87 +12 05 09.6 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 J089.8160+12.0897,2461128.6232,13.71,0.05,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
ATO J089.8160+12.0897 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:16.87 +12:05:09.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 51 37.51 +13 14 02.5 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
Gaia DR3 3346350346216685312,2461128.6232,13.84,0.05,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 3346350346216685312 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:37.51 +13:14:02.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.72 06:12:20.10 +10:02:03.9
199.52486 -3.97671 galactic Ori Second-epoch detections are separated by 1.8" and 2.9 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 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 29.1232* 06 12 20.10 +10 02 03.9 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 3329889454558446464,2461128.6232,13.72,0.05,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 3329889454558446464 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:20.10 +10:02:03.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.85 05:53:57.38 +15:58:38.5
192.13136 -4.98184 galactic Ori Second-epoch detections are separated by 3.1" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.4909+15.9780 | 05:53:57.38 +15:58:38.5 (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 29.1232* 05 53 57.38 +15 58 38.5 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
ATO J088.4909+15.9780,2461128.6232,13.85,0.05,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 J088.4909+15.9780 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:57.38 +15:58:38.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 10 55.23 +18 14 13.8 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6232,13.91,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:55.23 +18:14:13.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.91 05:58:27.39 +16:42:25.2
192.03711 -3.68221 galactic Ori Second-epoch detections are separated by 2.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.6120+16.6984 | 05:58:25.92 +16:42:00.2 (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 29.1232* 05 58 27.39 +16 42 25.2 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 J089.6120+16.6984,2461128.6232,13.91,0.05,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 J089.6120+16.6984 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:27.39 +16:42:25.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 54 00.73 +14 50 42.4 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,2461128.6232,13.88,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:00.73 +14:50:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.81 06:34:16.98 +17:15:29.9
195.63210 4.11291 galactic Gem Second-epoch detections are separated by 2.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:34:16.98 +17:15:29.9 (user input) | T | P | (position from user input) SpType: K5 (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,2461128.6232,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:16.98 +17:15:29.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 13 58.17 +14 27 25.2 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,2461128.6232,13.87,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:58.17 +14:27:25.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 13 27.44 +14 13 52.4 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 3344791960283157248,2461128.6232,13.82,0.05,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 3344791960283157248 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:27.44 +14:13:52.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 13 55.42 +12 05 34.8 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
ASASSN-V J061355.74+120554.2,2461128.6232,13.86,0.05,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
ASASSN-V J061355.74+120554.2 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:55.42 +12:05:34.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.76 06:29:40.32 +17:17:01.6
195.10341 3.14649 galactic Gem Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.4136+17.2758 | 06:29:40.32 +17:17:01.6 (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 J097.4136+17.2758,2461128.6232,13.76,0.05,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
ATO J097.4136+17.2758 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:29:40.32 +17:17:01.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.82 05:52:18.18 +15:51:58.7
192.02745 -5.38135 galactic Tau Second-epoch detections are separated by 0.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.0732+15.8575 | 05:52:18.18 +15:51:58.7 (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 29.1232* 05 52 18.18 +15 51 58.7 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+15.8575,2461128.6232,13.82,0.05,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 J088.0732+15.8575 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:18.18 +15:51:58.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 02 24.65 +14 17 47.4 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
Gaia DR3 3345361266787809536,2461128.6232,13.86,0.05,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
Gaia DR3 3345361266787809536 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:24.65 +14:17:47.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.63 06:24:13.84 +15:54:30.3
195.71650 1.35324 galactic Ori Second-epoch detections are separated by 1.9" and 2.9 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 J096.0574+15.9063 | 06:24:12.38 +15:54:21.9 (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 29.1232* 06 24 13.84 +15 54 30.3 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
ATO J096.0574+15.9063,2461128.6232,13.63,0.05,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 J096.0574+15.9063 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:24:13.84 +15:54:30.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.78 06:18:02.62 +17:41:17.8
193.44883 0.88426 galactic Ori Second-epoch detections are separated by 2.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J094.5060+17.6887 | 06:18:02.02 +17:41:29.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.960+/-0.184 (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 29.1232* 06 18 02.62 +17 41 17.8 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 J094.5060+17.6887,2461128.6232,13.78,0.05,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 J094.5060+17.6887 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:02.62 +17:41:17.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.84 06:38:34.20 +17:37:22.6
195.77184 5.18949 galactic Gem Second-epoch detections are separated by 2.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J099.6255+17.6319 | 06:38:32.93 +17:37:32.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J099.6255+17.6319,2461128.6232,13.84,0.05,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 J099.6255+17.6319 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:38:34.20 +17:37:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.88 05:54:41.60 +12:22:48.9
195.35558 -6.61965 galactic Ori Second-epoch detections are separated by 3.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.6778+12.3733 | 05:54:42.70 +12:22:24.0 (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 29.1232* 05 54 41.60 +12 22 48.9 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
ATO J088.6778+12.3733,2461128.6232,13.88,0.05,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 J088.6778+12.3733 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:41.60 +12:22:48.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.73 06:11:23.67 +14:49:43.7
195.19983 -1.88293 galactic Ori Second-epoch detections are separated by 1.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 11 23.67 +14 49 43.7 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
Gaia DR3 3345638137560150272,2461128.6232,13.73,0.05,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 3345638137560150272 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:23.67 +14:49:43.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.54 06:15:53.67 +14:10:16.5
196.29860 -1.24086 galactic Ori Second-epoch detections are separated by 1.2" and 2.9 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 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 29.1232* 06 15 53.67 +14 10 16.5 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 3344614114276769664,2461128.6232,13.54,0.05,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 3344614114276769664 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.54 06:13:49.73 +12:47:06.0
197.27843 -2.34303 galactic Ori Second-epoch detections are separated by 2.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 13 49.73 +12 47 06.0 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
Gaia DR3 3344068722150832640,2461128.6232,13.54,0.05,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 3344068722150832640 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:49.73 +12:47:06.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.82 05:55:31.07 +15:11:03.3
193.00962 -5.05243 galactic Ori Second-epoch detections are separated by 3.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 05 55 31.07 +15 11 03.3 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 J088.8872+15.1899,2461128.6232,13.82,0.05,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 J088.8872+15.1899 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:31.07 +15:11:03.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.65 06:09:12.84 +15:40:25.5
194.20547 -1.93648 galactic Ori Second-epoch detections are separated by 3.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3345947684442695168 | 06:09:12.84 +15:40:25.5 (user input) | DSCT/GDOR (local) | (local) | (position from user input) SpType: A0III (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 29.1232* 06 09 12.84 +15 40 25.5 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 3345947684442695168,2461128.6232,13.65,0.05,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 3345947684442695168 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:12.84 +15:40:25.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 51 38.55 +14 47 55.2 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 3347139177090170880,2461128.6232,13.77,0.05,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 3347139177090170880 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:38.55 +14:47:55.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.71 06:13:23.68 +17:13:26.6
193.32875 -0.31171 galactic Ori Second-epoch detections are separated by 3.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 13 23.68 +17 13 26.6 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 3370224798104166656,2461128.6232,13.71,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:23.68 +17:13:26.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.60 05:51:05.88 +15:39:53.7
192.05561 -5.73324 galactic Tau Second-epoch detections are separated by 2.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J087.7798+15.6708 | 05:51:05.88 +15:39:53.7 (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 29.1232* 05 51 05.88 +15 39 53.7 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 J087.7798+15.6708,2461128.6232,13.60,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:05.88 +15:39:53.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 00 53.36 +14 53 46.9 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 3348442785564417152,2461128.6232,13.66,0.05,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 3348442785564417152 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:53.36 +14:53:46.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 55 47.09 +14 33 50.9 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 3346976621168100608,2461128.6232,13.78,0.05,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
Gaia DR3 3346976621168100608 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:47.09 +14:33:50.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.60 06:00:25.20 +16:41:37.4
192.28192 -3.28031 galactic Ori Second-epoch detections are separated by 1.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.1078+16.6862 | 06:00:25.20 +16:41:37.4 (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 29.1232* 06 00 25.20 +16 41 37.4 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 J090.1078+16.6862,2461128.6232,13.60,0.05,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 J090.1078+16.6862 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:25.20 +16:41:37.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.46 06:27:09.44 +15:25:23.6
196.47444 1.75031 galactic Gem Second-epoch detections are separated by 2.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3356858310124918144 | 06:27:09.78 +15:24:59.6 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3356858310124918144,2461128.6232,13.46,0.05,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 3356858310124918144 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:09.44 +15:25:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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,2461128.6232,13.35,0.05,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 20260329.1232 13.35CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:38:45.68 +13:41:32.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.51 06:32:06.11 +18:09:37.2
194.58973 4.06319 galactic Gem Second-epoch detections are separated by 1.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:32:06.11 +18:09:37.2 (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,2461128.6232,13.51,0.05,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 20260329.1232 13.51CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:06.11 +18:09:37.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.46 06:13:48.73 +12:57:35.1
197.12281 -2.26319 galactic Ori Second-epoch detections are separated by 3.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3344084282812416768 | 06:13:49.92 +12:57:37.1 (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 29.1232* 06 13 48.73 +12 57 35.1 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 3344084282812416768,2461128.6232,13.46,0.05,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 3344084282812416768 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:48.73 +12:57:35.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 57 25.91 +11 32 51.5 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
Gaia DR3 3342940996877986944,2461128.6232,13.62,0.05,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 3342940996877986944 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:25.91 +11:32:51.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 14 38.16 +13 49 46.1 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 3344575631366615296,2461128.6232,13.38,0.05,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 3344575631366615296 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:38.16 +13:49:46.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 3355758935936342912,2461128.6232,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355758935936342912 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:39:55.14 +13:35:03.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 01 02.76 +13 48 59.6 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,2461128.6232,13.54,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:02.76 +13:48:59.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.13 06:35:42.69 +11:30:05.7
200.91520 1.78354 galactic Mon Second-epoch detections are separated by 1.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3328071270343378688 | 06:35:43.11 +11:29:45.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3328071270343378688,2461128.6232,13.13,0.05,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 3328071270343378688 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:42.69 +11:30:05.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.52 06:41:18.50 +18:02:07.2
195.69636 5.95704 galactic Gem Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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+18.0333,2461128.6232,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.3264+18.0333 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:18.50 +18:02:07.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.39 05:49:55.21 +12:51:44.4
194.34984 -7.38899 galactic Tau Second-epoch detections are separated by 2.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:49:55.21 +12:51:44.4 (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 29.1232* 05 49 55.21 +12 51 44.4 13.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6232,13.39,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:55.21 +12:51:44.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.14 06:31:42.82 +11:11:14.9
200.74248 0.76909 galactic Mon Second-epoch detections are separated by 2.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.9290+11.1885 | 06:31:41.88 +11:10:58.4 (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 J097.9290+11.1885,2461128.6232,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.9290+11.1885 20260329.1232 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:42.82 +11:11:14.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.42 06:36:11.37 +17:16:23.4
195.82669 4.52489 galactic Gem Second-epoch detections are separated by 2.3" and 2.9 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 3358966761109597952 | 06:36:12.78 +17:16:06.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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
Gaia DR3 3358966761109597952,2461128.6232,13.42,0.05,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 3358966761109597952 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:11.37 +17:16:23.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 55 57.28 +16 32 15.5 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
Gaia DR3 3349620942333555840,2461128.6232,13.55,0.05,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 3349620942333555840 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:57.28 +16:32:15.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.26 06:25:55.13 +15:51:16.3
195.95370 1.68710 galactic Gem Second-epoch detections are separated by 3.0" and 2.9 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 J096.4766+15.8569 | 06:25:55.13 +15:51:16.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J096.4766+15.8569,2461128.6232,13.26,0.05,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
ATO J096.4766+15.8569 20260329.1232 13.26CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:55.13 +15:51:16.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.19 06:40:48.75 +17:56:48.8
195.72268 5.81200 galactic Gem Second-epoch detections are separated by 1.9" and 2.9 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 3359474662462880896 | 06:40:49.92 +17:57:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3359474662462880896,2461128.6232,13.19,0.05,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 3359474662462880896 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:48.75 +17:56:48.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.37 06:26:36.81 +17:47:21.7
194.31685 2.73401 galactic Gem Second-epoch detections are separated by 2.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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+17.7948,2461128.6232,13.37,0.05,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
ATO J096.6559+17.7948 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:36.81 +17:47:21.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 49 25.37 +10 51 15.1 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
target,2461128.6232,13.20,0.05,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 20260329.1232 13.20CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:25.37 +10:51:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 50 34.10 +14 49 09.8 13.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6232,13.23,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:34.10 +14:49:09.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 3357736854275220864,2461128.6232,12.98,0.05,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
Gaia DR3 3357736854275220864 20260329.1232 12.98CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:51.58 +15:27:19.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 8.86 06:06:26.73 +10:44:52.7
198.20054 -4.90579 galactic Ori Second-epoch detections are separated by 1.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3330219445485837184 | 06:06:28.05 +10:45:00.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1958PMcCO..13b....V AG+10 687 J-Ks=0.236+/-0.033 (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!
TCP 2026 03 29.1232* 06 06 26.73 +10 44 52.7 8.9 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 3330219445485837184,2461128.6232,8.86,0.05,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
Gaia DR3 3330219445485837184 20260329.1232 8.86CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:26.73 +10:44:52.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 56 53.26 +14 50 24.2 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,2461128.6232,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.1232 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:53.26 +14:50:24.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 16 27.36 +16 42 37.2 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 3369945900107354240,2461128.6232,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3369945900107354240 20260329.1232 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:27.36 +16:42:37.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 12.89 06:03:45.61 +14:20:46.4
194.72649 -3.73252 galactic Ori Second-epoch detections are separated by 3.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:03:45.61 +14:20:46.4 (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 29.1232* 06 03 45.61 +14 20 46.4 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,2461128.6232,12.89,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:45.61 +14:20:46.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6232,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.1232 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:33.66 +17:55:15.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 12.97 06:16:45.41 +15:33:25.8
195.17844 -0.39843 galactic Ori Second-epoch detections are separated by 2.7" and 2.9 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 J094.1905+15.5509 | 06:16:47.72 +15:33:38.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1959ApJS....4...23M LF 8 +15 158
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 16 45.41 +15 33 25.8 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 J094.1905+15.5509,2461128.6232,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.1905+15.5509 20260329.1232 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:45.41 +15:33:25.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.09 06:10:12.01 +17:42:33.7
192.53684 -0.74619 galactic Ori Second-epoch detections are separated by 5.1" and 2.9 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 J092.5468+17.7042 | 06:10:12.01 +17:42:33.7 (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!
TCP 2026 03 29.1232* 06 10 12.01 +17 42 33.7 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+17.7042,2461128.6232,13.09,0.05,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
ATO J092.5468+17.7042 20260329.1232 13.09CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:12.01 +17:42:33.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.12 06:23:25.04 +17:30:59.4
194.20341 1.93316 galactic Gem Second-epoch detections are separated by 2.7" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3370435148423190656 | 06:23:25.03 +17:31:22.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3370435148423190656,2461128.6232,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3370435148423190656 20260329.1232 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:25.04 +17:30:59.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 19 42.39 +15 59 26.3 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,2461128.6232,13.06,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:42.39 +15:59:26.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.03 06:11:37.59 +13:51:44.9
196.07497 -2.29778 galactic Ori Second-epoch detections are separated by 3.4" and 2.9 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 J092.9138+13.8432 | 06:11:39.51 +13:51:18.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1959ApJS....4...23M LF 8 +13 89
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 11 37.59 +13 51 44.9 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 J092.9138+13.8432,2461128.6232,13.03,0.05,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 J092.9138+13.8432 20260329.1232 13.03CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:37.59 +13:51:44.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 08 41.20 +17 23 37.2 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
target,2461128.6232,13.21,0.05,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 20260329.1232 13.21CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:41.20 +17:23:37.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 13 09.91 +18 03 25.5 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
MGAB-V1815,2461128.6232,13.15,0.05,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
MGAB-V1815 20260329.1232 13.15CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:09.91 +18:03:25.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.19 06:05:30.91 +16:17:58.0
193.22614 -2.40978 galactic Ori Second-epoch detections are separated by 2.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3349024289775731584 | 06:05:31.66 +16:18:22.5 (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!
TCP 2026 03 29.1232* 06 05 30.91 +16 17 58.0 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 3349024289775731584,2461128.6232,13.19,0.05,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 3349024289775731584 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:30.91 +16:17:58.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.25 05:57:13.90 +17:30:31.9
191.19425 -3.53719 galactic Ori Second-epoch detections are separated by 1.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 05 57 13.90 +17 30 31.9 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 3349833182437442048,2461128.6232,13.25,0.05,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
Gaia DR3 3349833182437442048 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:13.90 +17:30:31.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.24 06:10:33.18 +17:47:20.1
192.50771 -0.63422 galactic Ori Second-epoch detections are separated by 5.6" and 2.5 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 J092.6385+17.7950 | 06:10:33.94 +17:47:36.7 (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!
TCP 2026 03 29.1232* 06 10 33.18 +17 47 20.1 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 J092.6385+17.7950,2461128.6232,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.6385+17.7950 20260329.1232 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:33.18 +17:47:20.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 57 47.60 +14 19 57.4 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,2461128.6232,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.1232 13.20CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:47.60 +14:19:57.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 17 11.15 +15 50 14.3 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 3369820933739293184,2461128.6232,13.20,0.05,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 3369820933739293184 20260329.1232 13.20CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:11.15 +15:50:14.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.37 05:56:44.14 +17:00:11.1
191.57441 -3.89204 galactic Ori Second-epoch detections are separated by 2.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 05 56 44.14 +17 00 11.1 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+17.0131,2461128.6232,13.37,0.05,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
ATO J089.1810+17.0131 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:44.14 +17:00:11.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.30 06:18:18.15 +14:22:19.4
196.39884 -0.63205 galactic Ori Second-epoch detections are separated by 2.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 18 18.15 +14 22 19.4 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 3344703621395907584,2461128.6232,13.30,0.05,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
Gaia DR3 3344703621395907584 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:18.15 +14:22:19.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.20 06:16:56.03 +15:17:01.8
195.43922 -0.49077 galactic Ori Second-epoch detections are separated by 2.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3345020246384468224 | 06:16:54.49 +15:17:17.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1959ApJS....4...23M LF 8 +15 161
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 16 56.03 +15 17 01.8 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 3345020246384468224,2461128.6232,13.20,0.05,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 3345020246384468224 20260329.1232 13.20CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:56.03 +15:17:01.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 10 55.69 +15 29 38.5 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
target,2461128.6232,13.25,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:55.69 +15:29:38.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 09 52.24 +11 19 55.0 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
EE Ori,2461128.6232,13.28,0.05,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
EE Ori 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:52.24 +11:19:55.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 3355237423827437568,2461128.6232,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3355237423827437568 20260329.1232 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:06.77 +12:37:58.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.24 06:37:54.50 +17:30:25.6
195.80401 4.99646 galactic Gem Second-epoch detections are separated by 2.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J099.4772+17.4939 | 06:37:54.54 +17:29:49.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J099.4772+17.4939,2461128.6232,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.4772+17.4939 20260329.1232 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:54.50 +17:30:25.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.27 06:20:46.44 +15:18:14.8
195.85947 0.33467 galactic Ori Second-epoch detections are separated by 1.6" and 2.9 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 | Large-amplitude variable Gaia DR2 3368795570423643520 | 06:20:48.44 +15:17:58.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: M0 1947AnDea...5....1L DO 12134
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 20 46.44 +15 18 14.8 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
Large-amplitude variable Gaia DR2 3368795570423643520,2461128.6232,13.27,0.05,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
Large-amplitude variable Gaia DR2 3368795570423643520 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:46.44 +15:18:14.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.39 06:22:11.62 +16:05:21.3
195.32730 1.00550 galactic Ori Second-epoch detections are separated by 2.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 22 11.62 +16 05 21.3 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 3369142569422792832,2461128.6232,13.39,0.05,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 3369142569422792832 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:11.62 +16:05:21.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.60 05:56:26.65 +17:40:49.6
190.95143 -3.61417 galactic Ori Second-epoch detections are separated by 3.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.1245+17.6814 | 05:56:28.59 +17:40:43.3 (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 29.1232* 05 56 26.65 +17 40 49.6 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 J089.1245+17.6814,2461128.6232,13.60,0.05,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 J089.1245+17.6814 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:26.65 +17:40:49.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.35 06:25:09.44 +15:58:53.2
195.75598 1.58431 galactic Ori Second-epoch detections are separated by 3.9" and 2.9 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 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 29.1232* 06 25 09.44 +15 58 53.2 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 3368959152842877696,2461128.6232,13.35,0.05,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
Gaia DR3 3368959152842877696 20260329.1232 13.35CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:09.44 +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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 07 01.07 +10 58 45.5 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 3330233872279561984,2461128.6232,13.29,0.05,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 3330233872279561984 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:01.07 +10:58:45.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 10 14.13 +13 48 21.8 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,2461128.6232,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:14.13 +13:48:21.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 02 06.73 +15 11 09.4 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,2461128.6232,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:06.73 +15:11:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 12 57.12 +17 26 20.6 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
ZTF J061257.09+172613.7,2461128.6232,13.41,0.05,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
ZTF J061257.09+172613.7 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:57.12 +17:26:20.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.30 06:17:52.61 +15:42:08.3
195.17869 -0.09220 galactic Ori Second-epoch detections are separated by 2.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J094.4766+15.7123 | 06:17:52.61 +15:42:08.3 (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 29.1232* 06 17 52.61 +15 42 08.3 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+15.7123,2461128.6232,13.30,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:52.61 +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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.55 05:57:12.71 +17:39:14.8
191.06575 -3.46886 galactic Ori Second-epoch detections are separated by 2.3" and 2.9 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 3350398297055720320 | 05:57:10.85 +17:39:53.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1931AnHar.100...61C HD 249535
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 57 12.71 +17 39 14.8 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
Gaia DR3 3350398297055720320,2461128.6232,13.55,0.05,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 3350398297055720320 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:12.71 +17:39:14.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.34 06:27:55.34 +17:41:36.1
194.54663 2.96568 galactic Gem Second-epoch detections are separated by 3.7" and 2.4 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 J096.9812+17.7016 | 06:27:55.49 +17:42:05.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0 (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 J096.9812+17.7016,2461128.6232,13.34,0.05,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
ATO J096.9812+17.7016 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:55.34 +17:41:36.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.37 06:06:27.04 +10:44:01.4
198.21368 -4.91155 galactic Ori Second-epoch detections are separated by 1.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.6122+10.7315 | 06:06:27.04 +10:44:01.4 (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 29.1232* 06 06 27.04 +10 44 01.4 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 J091.6122+10.7315,2461128.6232,13.37,0.05,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
ATO J091.6122+10.7315 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:27.04 +10:44:01.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.43 06:10:30.91 +14:52:41.1
195.05431 -2.04550 galactic Ori Second-epoch detections are separated by 1.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 10 30.91 +14 52 41.1 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 3345637484724562688,2461128.6232,13.43,0.05,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 3345637484724562688 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:30.91 +14:52:41.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 12 28.10 +15 20 03.5 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
target,2461128.6232,13.41,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:28.10 +15:20:03.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.32 06:29:40.10 +11:43:01.9
200.04089 0.57009 galactic Mon Second-epoch detections are separated by 4.5" and 2.4 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 J097.4148+11.7101 | 06:29:40.10 +11:43:01.9 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J097.4148+11.7101,2461128.6232,13.32,0.05,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
ATO J097.4148+11.7101 20260329.1232 13.32CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:29:40.10 +11:43:01.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.45 06:07:20.22 +16:45:35.4
193.03647 -1.80424 galactic Ori Second-epoch detections are separated by 3.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3349202956117251072 | 06:07:17.82 +16:46:05.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.752+/-0.275 (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 29.1232* 06 07 20.22 +16 45 35.4 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 3349202956117251072,2461128.6232,13.45,0.05,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 3349202956117251072 20260329.1232 13.45CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:20.22 +16:45:35.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 14 37.25 +16 02 29.7 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
target,2461128.6232,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:37.25 +16:02:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.41 06:38:54.79 +15:11:20.6
197.98656 4.16075 galactic Gem Second-epoch detections are separated by 5.1" and 2.4 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 | 06:38:54.79 +15:11:20.6 (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,2461128.6232,13.41,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:38:54.79 +15:11:20.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.46 05:54:13.85 +13:11:37.5
194.58850 -6.31380 galactic Ori Second-epoch detections are separated by 2.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.5475+13.1904 | 05:54:13.85 +13:11:37.5 (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 29.1232* 05 54 13.85 +13 11 37.5 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
ATO J088.5475+13.1904,2461128.6232,13.46,0.05,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 J088.5475+13.1904 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:13.85 +13:11:37.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.48 06:35:02.86 +17:42:00.9
195.32095 4.47663 galactic Gem Second-epoch detections are separated by 4.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3371007817883953024 | 06:35:03.66 +17:41:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3371007817883953024,2461128.6232,13.48,0.05,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 3371007817883953024 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:02.86 +17:42:00.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.58 05:56:33.25 +15:11:30.2
193.12802 -4.83184 galactic Ori Second-epoch detections are separated by 3.0" and 2.9 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 3347211951016560512 | 05:56:31.43 +15:11:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 56 33.25 +15 11 30.2 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 3347211951016560512,2461128.6232,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3347211951016560512 20260329.1232 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:33.25 +15:11:30.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 202090420,2461128.6232,13.45,0.05,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
EPIC 202090420 20260329.1232 13.45CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:05.27 +17:47:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.56 06:27:44.25 +17:39:43.5
194.55399 2.91218 galactic Gem Second-epoch detections are separated by 3.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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+17.6679,2461128.6232,13.56,0.05,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 J096.9262+17.6679 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:44.25 +17:39:43.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.48 06:19:14.38 +17:25:24.8
193.81697 1.01018 galactic Ori Second-epoch detections are separated by 2.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3370096838139971840 | 06:19:13.69 +17:26:03.1 (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 29.1232* 06 19 14.38 +17 25 24.8 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 3370096838139971840,2461128.6232,13.48,0.05,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 3370096838139971840 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:14.38 +17:25:24.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.48 06:16:19.85 +14:31:16.3
196.04101 -0.98143 galactic Ori Second-epoch detections are separated by 3.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 16 19.85 +14 31 16.3 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 3344815324905336320,2461128.6232,13.48,0.05,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 3344815324905336320 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:19.85 +14:31:16.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.48 05:54:35.46 +12:10:02.2
195.52939 -6.74686 galactic Ori Second-epoch detections are separated by 2.5" and 2.9 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 3343222441794756608 | 05:54:32.50 +12:09:47.9 (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 29.1232* 05 54 35.46 +12 10 02.2 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 3343222441794756608,2461128.6232,13.48,0.05,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 3343222441794756608 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:35.46 +12:10:02.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.47 06:00:20.47 +15:32:27.5
193.27705 -3.86578 galactic Ori Second-epoch detections are separated by 2.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 00 20.47 +15 32 27.5 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
ATO J090.0761+15.5386,2461128.6232,13.47,0.05,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 J090.0761+15.5386 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:20.47 +15:32:27.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.59 05:59:54.86 +17:17:28.4
191.70192 -3.08990 galactic Ori Second-epoch detections are separated by 3.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3350141835968703744 | 05:59:53.56 +17:17:52.9 (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 29.1232* 05 59 54.86 +17 17 28.4 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
Gaia DR3 3350141835968703744,2461128.6232,13.59,0.05,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
Gaia DR3 3350141835968703744 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:54.86 +17:17:28.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.46 06:14:42.27 +15:10:59.5
195.27162 -1.01156 galactic Ori Second-epoch detections are separated by 2.3" and 2.9 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 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 29.1232* 06 14 42.27 +15 10 59.5 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 3345004097307291776,2461128.6232,13.46,0.05,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 3345004097307291776 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:42.27 +15:10:59.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.49 05:58:48.35 +13:38:11.6
194.75531 -5.12794 galactic Ori Second-epoch detections are separated by 1.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 05 58 48.35 +13 38 11.6 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 3343853149152246784,2461128.6232,13.49,0.05,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
Gaia DR3 3343853149152246784 20260329.1232 13.49CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:48.35 +13:38:11.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.81 05:57:00.05 +17:55:40.0
190.80305 -3.37585 galactic Ori Second-epoch detections are separated by 3.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:57:00.05 +17:55:40.0 (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 29.1232* 05 57 00.05 +17 55 40.0 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
target,2461128.6232,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:00.05 +17:55:40.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.51 06:34:47.09 +15:31:01.1
197.23949 3.42428 galactic Gem Second-epoch detections are separated by 1.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 3357086385767980544,2461128.6232,13.51,0.05,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
Gaia DR3 3357086385767980544 20260329.1232 13.51CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:47.09 +15:31:01.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.52 06:15:28.00 +14:23:53.4
196.04965 -1.22397 galactic Ori Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 15 28.00 +14 23 53.4 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 3344809827347251968,2461128.6232,13.52,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:28.00 +14:23:53.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 54 30.48 +12 57 30.9 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
target,2461128.6232,13.69,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:30.48 +12:57:30.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.60 06:20:57.18 +16:50:14.0
194.52717 1.09463 galactic Ori Second-epoch detections are separated by 2.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 20 57.18 +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+16.8424,2461128.6232,13.60,0.05,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 J095.2326+16.8424 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:57.18 +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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.64 06:31:32.15 +18:03:36.5
194.61724 3.89774 galactic Gem Second-epoch detections are separated by 2.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.8827+18.0771 | 06:31:31.88 +18:04:12.7 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J097.8827+18.0771,2461128.6232,13.64,0.05,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 J097.8827+18.0771 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:32.15 +18:03:36.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.51 06:11:37.15 +15:28:26.2
194.65992 -1.52529 galactic Ori Second-epoch detections are separated by 2.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 11 37.15 +15 28 26.2 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 3345733966869577344,2461128.6232,13.51,0.05,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
Gaia DR3 3345733966869577344 20260329.1232 13.51CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:37.15 +15:28:26.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.70 05:54:22.03 +15:30:54.7
192.58270 -5.12760 galactic Ori Second-epoch detections are separated by 1.7" and 2.9 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 J088.5882+15.5137 | 05:54:20.87 +15:31:05.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 54 22.03 +15 30 54.7 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
ATO J088.5882+15.5137,2461128.6232,13.70,0.05,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
ATO J088.5882+15.5137 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:22.03 +15:30:54.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 49 14.20 +14 41 49.7 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 3347873341620021248,2461128.6232,13.79,0.05,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 3347873341620021248 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:14.20 +14:41:49.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.80 05:58:26.34 +15:59:27.6
192.65812 -4.04105 galactic Ori Second-epoch detections are separated by 2.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 05 58 26.34 +15 59 27.6 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 3348824934574492416,2461128.6232,13.80,0.05,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 3348824934574492416 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:26.34 +15:59:27.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.66 06:19:47.07 +16:38:51.9
194.56241 0.75861 galactic Ori Second-epoch detections are separated by 1.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 19 47.07 +16 38 51.9 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
ATO J094.9454+16.6480,2461128.6232,13.66,0.05,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 J094.9454+16.6480 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:47.07 +16:38:51.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 57 13.12 +12 48 33.4 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
ASASSN-V J055711.94+124843.4,2461128.6232,13.61,0.05,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
ASASSN-V J055711.94+124843.4 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:13.12 +12:48:33.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.55 06:06:58.48 +14:36:07.9
194.88190 -2.92821 galactic Ori Second-epoch detections are separated by 3.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.7404+14.6020 | 06:06:58.48 +14:36:07.9 (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 29.1232* 06 06 58.48 +14 36 07.9 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
ATO J091.7404+14.6020,2461128.6232,13.55,0.05,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 J091.7404+14.6020 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:58.48 +14:36:07.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.68 06:12:31.18 +15:20:12.7
194.88446 -1.40074 galactic Ori Second-epoch detections are separated by 2.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J093.1411+15.3416 | 06:12:31.18 +15:20:12.7 (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 29.1232* 06 12 31.18 +15 20 12.7 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
ATO J093.1411+15.3416,2461128.6232,13.68,0.05,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 J093.1411+15.3416 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:31.18 +15:20:12.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 03 52.36 +14 59 05.9 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 3345547457913147008,2461128.6232,13.65,0.05,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 3345547457913147008 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:52.36 +14:59:05.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.61 06:18:54.41 +11:33:57.4
198.94154 -1.82948 galactic Ori Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 18 54.41 +11 33 57.4 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 J094.7333+11.5622,2461128.6232,13.61,0.05,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
ATO J094.7333+11.5622 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:54.41 +11:33:57.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.53 06:21:38.01 +12:02:48.8
198.83167 -1.01434 galactic Ori Second-epoch detections are separated by 3.7" and 2.9 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 J095.4093+12.0449 | 06:21:40.05 +12:02:57.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3 1959ApJS....4...23M LF 8 +12 286
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 21 38.01 +12 02 48.8 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
ATO J095.4093+12.0449,2461128.6232,13.53,0.05,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 J095.4093+12.0449 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:38.01 +12:02:48.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.75 05:49:28.23 +11:30:41.3
195.47486 -8.15997 galactic Ori Second-epoch detections are separated by 1.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 05 49 28.23 +11 30 41.3 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 3337087682306216192,2461128.6232,13.75,0.05,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 3337087682306216192 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:28.23 +11:30:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.73 06:12:26.70 +15:00:24.4
195.16554 -1.57487 galactic Ori Second-epoch detections are separated by 2.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J093.1120+15.0101 | 06:12:26.70 +15:00:24.4 (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 29.1232* 06 12 26.70 +15 00 24.4 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
ATO J093.1120+15.0101,2461128.6232,13.73,0.05,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
ATO J093.1120+15.0101 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:26.70 +15:00:24.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.64 06:02:32.64 +14:05:00.5
194.81182 -4.11808 galactic Ori Second-epoch detections are separated by 2.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3345336596495908864 | 06:02:30.71 +14:04:48.8 (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 29.1232* 06 02 32.64 +14 05 00.5 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
Gaia DR3 3345336596495908864,2461128.6232,13.64,0.05,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
Gaia DR3 3345336596495908864 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:32.64 +14:05:00.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 04 53.18 +10 54 04.3 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
Gaia DR3 3341863956521497088,2461128.6232,13.63,0.05,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
Gaia DR3 3341863956521497088 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:53.18 +10:54:04.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.74 05:57:33.73 +15:38:38.1
192.85538 -4.39636 galactic Ori Second-epoch detections are separated by 1.7" and 2.9 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 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 29.1232* 05 57 33.73 +15 38 38.1 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
ATO J089.3854+15.6467,2461128.6232,13.74,0.05,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 J089.3854+15.6467 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:33.73 +15:38:38.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.72 06:10:46.67 +14:47:19.1
195.16334 -2.03293 galactic Ori Second-epoch detections are separated by 4.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.6913+14.7916 | 06:10:46.67 +14:47:19.1 (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 29.1232* 06 10 46.67 +14 47 19.1 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
ATO J092.6913+14.7916,2461128.6232,13.72,0.05,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 J092.6913+14.7916 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:46.67 +14:47:19.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.71 05:48:53.22 +10:13:09.7
196.53548 -8.92808 galactic Ori Second-epoch detections are separated by 3.7" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:48:53.22 +10:13:09.7 (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 29.1232* 05 48 53.22 +10 13 09.7 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,2461128.6232,13.71,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.22 +10:13:09.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 56 30.04 +12 01 33.2 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
ZTF J055630.04+120126.8,2461128.6232,13.76,0.05,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
ZTF J055630.04+120126.8 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:30.04 +12:01:33.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 07 36.39 +10 59 23.3 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,2461128.6232,13.65,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:36.39 +10:59:23.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 50 55.72 +13 52 50.5 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,2461128.6232,13.65,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:55.72 +13:52:50.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 19 12.12 +12 45 05.8 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
Gaia DR3 3332386995222063616,2461128.6232,13.59,0.05,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
Gaia DR3 3332386995222063616 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:12.12 +12:45:05.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.61 06:41:44.73 +15:13:17.5
198.26780 4.78471 galactic Gem Second-epoch detections are separated by 3.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J100.4280+15.2323 | 06:41:43.39 +15:13:34.5 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.4280+15.2323,2461128.6232,13.61,0.05,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
ATO J100.4280+15.2323 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:44.73 +15:13:17.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.79 06:23:49.23 +16:28:13.4
195.17355 1.52900 galactic Ori Second-epoch detections are separated by 4.7" and 2.5 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 | 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 29.1232* 06 23 49.23 +16 28 13.4 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
EPIC 202083480,2461128.6232,13.79,0.05,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
EPIC 202083480 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:49.23 +16:28:13.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.71 06:11:05.87 +16:19:10.2
193.85812 -1.22839 galactic Ori Second-epoch detections are separated by 4.9" and 2.4 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 | 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 29.1232* 06 11 05.87 +16 19 10.2 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
EG Ori,2461128.6232,13.71,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:05.87 +16:19:10.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.75 05:50:50.16 +14:25:32.6
193.10035 -6.41173 galactic Tau Second-epoch detections are separated by 3.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:50:50.16 +14:25:32.6 (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 29.1232* 05 50 50.16 +14 25 32.6 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
target,2461128.6232,13.75,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:50.16 +14:25:32.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.76 06:01:37.66 +14:43:11.3
194.14675 -3.99956 galactic Ori Second-epoch detections are separated by 2.0" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 01 37.66 +14 43 11.3 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 3345434448731575424,2461128.6232,13.76,0.05,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 3345434448731575424 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:37.66 +14:43:11.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.79 05:55:56.95 +15:40:28.5
192.63495 -4.71795 galactic Ori Second-epoch detections are separated by 2.1" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3348785833192100608 | 05:55:58.08 +15:39:56.6 (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!
TCP 2026 03 29.1232* 05 55 56.95 +15 40 28.5 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 3348785833192100608,2461128.6232,13.79,0.05,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 3348785833192100608 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:56.95 +15:40:28.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.82 05:56:21.65 +17:58:16.6
190.68912 -3.48598 galactic Ori Second-epoch detections are separated by 3.1" and 2.9 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 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 29.1232* 05 56 21.65 +17 58 16.6 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 3350422147011829760,2461128.6232,13.82,0.05,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 3350422147011829760 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:21.65 +17:58:16.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 20 58.57 +14 41 22.8 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
ASASSN-V J062058.41+144114.8,2461128.6232,13.65,0.05,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
ASASSN-V J062058.41+144114.8 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:58.57 +14:41:22.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 58 16.45 +16 05 42.7 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 3348826510825019392,2461128.6232,13.82,0.05,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 3348826510825019392 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:16.45 +16:05:42.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.70 05:48:53.57 +10:23:25.0
196.38614 -8.84181 galactic Ori Second-epoch detections are separated by 3.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J087.2226+10.3883 | 05:48:54.01 +10:22:46.2 (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 29.1232* 05 48 53.57 +10 23 25.0 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 J087.2226+10.3883,2461128.6232,13.70,0.05,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
ATO J087.2226+10.3883 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.57 +10:23:25.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.82 05:58:03.65 +15:30:43.4
193.02996 -4.35751 galactic Ori Second-epoch detections are separated by 2.5" and 2.9 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 3348724260541283712 | 05:58:05.32 +15:30:47.5 (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 29.1232* 05 58 03.65 +15 30 43.4 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 3348724260541283712,2461128.6232,13.82,0.05,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 3348724260541283712 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:03.65 +15:30:43.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.84 06:26:05.78 +16:32:36.8
195.36344 2.04563 galactic Gem Second-epoch detections are separated by 3.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.5229+16.5449 | 06:26:04.00 +16:32:41.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J096.5229+16.5449,2461128.6232,13.84,0.05,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 J096.5229+16.5449 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:05.78 +16:32:36.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.56 06:18:06.36 +11:26:20.6
198.96068 -2.06234 galactic Ori Second-epoch detections are separated by 2.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3331593869380208512 | 06:18:07.82 +11:26:29.7 (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 29.1232* 06 18 06.36 +11 26 20.6 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 3331593869380208512,2461128.6232,13.56,0.05,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
Gaia DR3 3331593869380208512 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:06.36 +11:26:20.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.73 06:25:59.18 +14:56:44.5
196.76568 1.27799 galactic Gem Second-epoch detections are separated by 2.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.5043+14.9344 | 06:25:59.65 +14:56:13.4 (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 J096.5043+14.9344,2461128.6232,13.73,0.05,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
ATO J096.5043+14.9344 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:59.18 +14:56:44.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.79 06:12:49.42 +11:40:07.8
198.14295 -3.09165 galactic Ori Second-epoch detections are separated by 2.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J061251.78+114014.2 | 06:12:51.00 +11:40:07.5 (Gaia DR3) | ROT (local) | 2.28725 (local) | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 12 49.42 +11 40 07.8 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
ASASSN-V J061251.78+114014.2,2461128.6232,13.79,0.05,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
ASASSN-V J061251.78+114014.2 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:49.42 +11:40:07.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.74 06:09:15.54 +11:12:53.5
198.12324 -4.07584 galactic Ori Second-epoch detections are separated by 3.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3330252430834705408 | 06:09:17.01 +11:12:32.4 (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 29.1232* 06 09 15.54 +11 12 53.5 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 3330252430834705408,2461128.6232,13.74,0.05,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 3330252430834705408 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:15.54 +11:12:53.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.80 06:05:26.55 +12:45:45.3
196.31262 -4.14623 galactic Ori Second-epoch detections are separated by 3.0" and 2.9 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 3342763631908993536 | 06:05:27.81 +12:45:11.0 (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 29.1232* 06 05 26.55 +12 45 45.3 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 3342763631908993536,2461128.6232,13.80,0.05,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 3342763631908993536 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:26.55 +12:45:45.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.83 06:00:57.42 +16:27:52.8
192.54507 -3.28148 galactic Ori Second-epoch detections are separated by 3.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 00 57.42 +16 27 52.8 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 3348915644282911488,2461128.6232,13.83,0.05,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 3348915644282911488 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:57.42 +16:27:52.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 57 34.57 +11 12 21.5 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 3342086577562180224,2461128.6232,13.80,0.05,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 3342086577562180224 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:34.57 +11:12:21.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.84 06:11:09.02 +17:31:04.6
192.81373 -0.64018 galactic Ori Second-epoch detections are separated by 2.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 11 09.02 +17 31 04.6 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
Large-amplitude variable Gaia DR2 3373230450575549696,2461128.6232,13.84,0.05,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
Large-amplitude variable Gaia DR2 3373230450575549696 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:09.02 +17:31:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 13 14.11 +13 29 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 3344188156600778368,2461128.6232,13.74,0.05,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 3344188156600778368 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:14.11 +13:29:52.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.75 05:50:37.80 +12:00:50.3
195.17828 -7.66323 galactic Ori Second-epoch detections are separated by 0.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3343162479753900800 | 05:50:37.90 +12:00:07.5 (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 29.1232* 05 50 37.80 +12 00 50.3 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 3343162479753900800,2461128.6232,13.75,0.05,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 3343162479753900800 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:37.80 +12:00:50.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.66 06:28:04.93 +14:04:45.4
197.76886 1.32386 galactic Gem Second-epoch detections are separated by 3.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.0245+14.0837 | 06:28:05.89 +14:05:01.4 (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 J097.0245+14.0837,2461128.6232,13.66,0.05,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 J097.0245+14.0837 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:04.93 +14:04:45.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 51 00.49 +13 29 08.0 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 3346439269219001472,2461128.6232,13.85,0.05,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 3346439269219001472 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:00.49 +13:29:08.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.89 06:19:04.28 +16:47:19.9
194.35736 0.67477 galactic Ori Second-epoch detections are separated by 2.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 19 04.28 +16 47 19.9 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
ATO J094.7664+16.8094,2461128.6232,13.89,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:04.28 +16:47:19.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.96 06:05:37.30 +17:10:43.6
192.47050 -1.95844 galactic Ori Second-epoch detections are separated by 2.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.4017+17.1781 | 06:05:37.30 +17:10:43.6 (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 29.1232* 06 05 37.30 +17 10 43.6 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 J091.4017+17.1781,2461128.6232,13.96,0.05,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
ATO J091.4017+17.1781 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:37.30 +17:10:43.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.76 05:53:09.28 +11:49:52.4
195.64804 -7.21849 galactic Ori Second-epoch detections are separated by 2.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.2911+11.8307 | 05:53:09.28 +11:49:52.4 (user input) | dubious (ATLAS) | (ATLAS) | (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 29.1232* 05 53 09.28 +11 49 52.4 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 J088.2911+11.8307,2461128.6232,13.76,0.05,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
ATO J088.2911+11.8307 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:09.28 +11:49:52.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.76 06:14:02.40 +15:01:15.6
195.33752 -1.22994 galactic Ori Second-epoch detections are separated by 1.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3344907026748313344 | 06:14:00.86 +15:01:36.0 (Gaia DR3) | T | P | 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 29.1232* 06 14 02.40 +15 01 15.6 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 3344907026748313344,2461128.6232,13.76,0.05,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 3344907026748313344 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:02.40 +15:01:15.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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,2461128.6232,13.86,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:29:32.69 +17:39:52.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.82 05:50:32.94 +15:45:58.9
191.90058 -5.79613 galactic Tau Second-epoch detections are separated by 3.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3348089773612051072 | 05:50:31.88 +15:46:21.2 (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 29.1232* 05 50 32.94 +15 45 58.9 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 3348089773612051072,2461128.6232,13.82,0.05,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 3348089773612051072 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:32.94 +15:45:58.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.74 06:12:18.19 +15:12:21.7
194.97423 -1.50932 galactic Ori Second-epoch detections are separated by 1.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 12 18.19 +15 12 21.7 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
ATO J093.0787+15.2153,2461128.6232,13.74,0.05,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 J093.0787+15.2153 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:18.19 +15:12:21.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 13 16.49 +15 43 24.4 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 3345836668127142784,2461128.6232,13.78,0.05,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
Gaia DR3 3345836668127142784 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:16.49 +15:43:24.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.82 06:25:40.26 +17:47:38.4
194.20839 2.53749 galactic Gem Second-epoch detections are separated by 3.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.4133+17.8001 | 06:25:40.26 +17:47:38.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J096.4133+17.8001,2461128.6232,13.82,0.05,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 J096.4133+17.8001 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:40.26 +17:47:38.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 09 55.66 +14 26 06.5 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
target,2461128.6232,13.83,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:55.66 +14:26:06.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.94 06:01:34.55 +16:08:07.9
192.90525 -3.31444 galactic Ori Second-epoch detections are separated by 3.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3348885545152160128 | 06:01:32.66 +16:08:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1931AnHar.100...61C HD 250458
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 01 34.55 +16 08 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
Gaia DR3 3348885545152160128,2461128.6232,13.94,0.05,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 3348885545152160128 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:34.55 +16:08:07.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.71 06:02:46.01 +11:05:17.8
197.46266 -5.53133 galactic Ori Second-epoch detections are separated by 1.5" and 2.9 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 | 06:02:46.01 +11:05:17.8 (user input) | T | P | (position from user input) J-Ks=0.546+/-0.306 (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 29.1232* 06 02 46.01 +11 05 17.8 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
target,2461128.6232,13.71,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:46.01 +11:05:17.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.06 05:59:14.13 +16:16:41.1
192.50316 -3.73266 galactic Ori Second-epoch detections are separated by 2.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:59:14.13 +16:16:41.1 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 59 14.13 +16 16 41.1 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,2461128.6232,14.06,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:14.13 +16:16:41.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.98 06:19:02.10 +16:47:08.2
194.35611 0.66557 galactic Ori Second-epoch detections are separated by 1.8" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 19 02.10 +16 47 08.2 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 J094.7504+16.7831,2461128.6232,13.98,0.05,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 J094.7504+16.7831 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:02.10 +16:47:08.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.10 05:51:57.97 +14:40:17.5
193.02469 -6.05179 galactic Tau Second-epoch detections are separated by 3.3" and 2.9 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 J087.9875+14.6525 | 05:51:56.94 +14:39:44.7 (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!
TCP 2026 03 29.1232* 05 51 57.97 +14 40 17.5 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 J087.9875+14.6525,2461128.6232,14.10,0.05,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 J087.9875+14.6525 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:57.97 +14:40:17.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 50 16.03 +13 54 05.4 14.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6232,14.04,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:16.03 +13:54:05.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 53 56.26 +15 51 26.8 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 3349557862154343168,2461128.6232,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3349557862154343168 20260329.1232 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:56.26 +15:51:26.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 3369382602261570688,2461128.6232,13.85,0.05,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 3369382602261570688 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:51.81 +16:41:07.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.93 05:53:13.27 +14:40:26.4
193.17543 -5.78788 galactic Ori Second-epoch detections are separated by 2.7" and 2.9 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 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 29.1232* 05 53 13.27 +14 40 26.4 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
Gaia DR3 3347084712605690112,2461128.6232,13.93,0.05,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
Gaia DR3 3347084712605690112 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:13.27 +14:40:26.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.05 05:51:52.97 +15:55:28.7
191.92575 -5.43930 galactic Tau Second-epoch detections are separated by 1.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3348113997229137024 | 05:51:52.33 +15:56:00.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1931AnHar.100...61C HD 248514
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 51 52.97 +15 55 28.7 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
Gaia DR3 3348113997229137024,2461128.6232,14.05,0.05,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 3348113997229137024 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:52.97 +15:55:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.90 06:16:58.71 +18:09:12.0
192.91918 0.88179 galactic Ori Second-epoch detections are separated by 2.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 16 58.71 +18 09 12.0 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 J094.2473+18.1622,2461128.6232,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.2473+18.1622 20260329.1232 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:58.71 +18:09:12.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 17 35.48 +14 21 38.5 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
target,2461128.6232,13.87,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:35.48 +14:21:38.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.71 06:26:03.55 +16:32:25.5
195.36208 2.03629 galactic Gem Second-epoch detections are separated by 3.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.5229+16.5449 | 06:26:04.00 +16:32:41.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J096.5229+16.5449,2461128.6232,13.71,0.05,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
ATO J096.5229+16.5449 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:03.55 +16:32:25.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 01 33.58 +16 49 51.0 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,2461128.6232,13.95,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:33.58 +16:49:51.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 18 42.38 +17 53 59.0 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 3370685733996143616,2461128.6232,13.96,0.05,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 3370685733996143616 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:42.38 +17:53:59.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.88 06:20:51.87 +17:05:08.9
194.29784 1.19298 galactic Ori Second-epoch detections are separated by 4.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3370025752140122752 | 06:20:51.86 +17:05:33.2 (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 29.1232* 06 20 51.87 +17 05 08.9 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 3370025752140122752,2461128.6232,13.88,0.05,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 3370025752140122752 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:51.87 +17:05:08.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.13 05:52:58.21 +15:17:40.7
192.60511 -5.52949 galactic Tau Second-epoch detections are separated by 1.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3347263353184496768 | 05:52:55.71 +15:17:40.7 (Gaia DR3) | T | P | 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 29.1232* 05 52 58.21 +15 17 40.7 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
Gaia DR3 3347263353184496768,2461128.6232,14.13,0.05,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 3347263353184496768 20260329.1232 14.13CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:58.21 +15:17:40.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.90 06:06:48.58 +16:40:37.3
193.04744 -1.95484 galactic Ori Second-epoch detections are separated by 2.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 06 48.58 +16 40 37.3 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 J091.7202+16.6787,2461128.6232,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.7202+16.6787 20260329.1232 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:48.58 +16:40:37.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.91 06:11:58.99 +17:22:43.8
193.03127 -0.53300 galactic Ori Second-epoch detections are separated by 2.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 11 58.99 +17 22 43.8 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 3373213305067527296,2461128.6232,13.91,0.05,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 3373213305067527296 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:58.99 +17:22:43.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.01 05:56:29.76 +15:23:10.1
192.95176 -4.74734 galactic Ori Second-epoch detections are separated by 2.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.1277+15.3906 | 05:56:30.06 +15:23:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 56 29.76 +15 23 10.1 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 J089.1277+15.3906,2461128.6232,14.01,0.05,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 J089.1277+15.3906 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:29.76 +15:23:10.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 14 08.37 +17 22 59.0 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
target,2461128.6232,13.85,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:08.37 +17:22:59.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.01 05:56:56.29 +16:55:37.5
191.66464 -3.88796 galactic Ori Second-epoch detections are separated by 1.7" and 2.9 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 3349774564723838976 | 05:56:54.29 +16:55:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 29.1232* 05 56 56.29 +16 55 37.5 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 3349774564723838976,2461128.6232,14.01,0.05,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 3349774564723838976 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:56.29 +16:55:37.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.94 05:59:56.14 +11:30:33.4
196.75321 -5.93219 galactic Ori Second-epoch detections are separated by 3.1" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 05 59 56.14 +11 30 33.4 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
Gaia DR3 3342200617534182784,2461128.6232,13.94,0.05,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 3342200617534182784 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:56.14 +11:30:33.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.02 06:01:42.15 +16:14:30.0
192.82770 -3.23572 galactic Ori Second-epoch detections are separated by 2.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:01:42.15 +16:14:30.0 (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 29.1232* 06 01 42.15 +16 14 30.0 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
target,2461128.6232,14.02,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:42.15 +16:14:30.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.12 05:55:47.25 +14:48:04.2
193.37572 -5.18670 galactic Ori Second-epoch detections are separated by 5.0" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.9441+14.8079 | 05:55:47.25 +14:48:04.2 (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 29.1232* 05 55 47.25 +14 48 04.2 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 J088.9441+14.8079,2461128.6232,14.12,0.05,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 J088.9441+14.8079 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:47.25 +14:48:04.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 14 35.32 +13 49 52.5 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
target,2461128.6232,13.73,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:35.32 +13:49:52.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.96 06:18:28.87 +14:20:26.5
196.44696 -0.60878 galactic Ori Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:18:28.87 +14:20:26.5 (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 29.1232* 06 18 28.87 +14 20 26.5 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
target,2461128.6232,13.96,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:28.87 +14:20:26.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.93 06:06:22.14 +14:21:40.1
195.02170 -3.17339 galactic Ori Second-epoch detections are separated by 3.2" and 2.9 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 J091.5792+14.3636 | 06:06:22.14 +14:21:40.1 (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 29.1232* 06 06 22.14 +14 21 40.1 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
ATO J091.5792+14.3636,2461128.6232,13.93,0.05,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 J091.5792+14.3636 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:22.14 +14:21:40.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 00 22.07 +10 05 27.1 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
VARIABLE_NAME,2461128.6232,13.76,0.05,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
VARIABLE_NAME 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:22.07 +10:05:27.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.78 06:18:52.50 +13:48:26.1
196.96213 -0.77705 galactic Ori Second-epoch detections are separated by 4.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J094.7197+13.7963 | 06:18:52.50 +13:48:26.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 18 52.50 +13 48 26.1 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 J094.7197+13.7963,2461128.6232,13.78,0.05,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 J094.7197+13.7963 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:18:52.50 +13:48:26.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.87 06:05:27.21 +10:56:04.5
197.91848 -5.02905 galactic Ori Second-epoch detections are separated by 3.7" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3342238821267200000 | 06:05:28.60 +10:55:44.0 (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 29.1232* 06 05 27.21 +10 56 04.5 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 3342238821267200000,2461128.6232,13.87,0.05,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 3342238821267200000 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:27.21 +10:56:04.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.93 06:11:38.95 +16:33:10.4
193.71712 -1.00019 galactic Ori Second-epoch detections are separated by 2.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3346143702450969472 | 06:11:37.23 +16:33:17.4 (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 29.1232* 06 11 38.95 +16 33 10.4 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
Gaia DR3 3346143702450969472,2461128.6232,13.93,0.05,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
Gaia DR3 3346143702450969472 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:38.95 +16:33:10.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.84 06:39:09.96 +13:11:14.6
199.80095 3.30492 galactic Gem Second-epoch detections are separated by 1.0" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J099.7912+13.1850 | 06:39:09.96 +13:11:14.6 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J099.7912+13.1850,2461128.6232,13.84,0.05,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 J099.7912+13.1850 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:39:09.96 +13:11:14.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.93 06:01:17.73 +15:06:07.6
193.77346 -3.88161 galactic Ori Second-epoch detections are separated by 3.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3348482058746163456 | 06:01:15.41 +15:05:54.8 (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 29.1232* 06 01 17.73 +15 06 07.6 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 3348482058746163456,2461128.6232,13.93,0.05,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
Gaia DR3 3348482058746163456 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:17.73 +15:06:07.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.95 06:16:11.26 +14:06:20.4
196.39012 -1.20955 galactic Ori Second-epoch detections are separated by 4.3" and 2.5 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 3344609716230257920 | 06:16:11.69 +14:05:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 16 11.26 +14 06 20.4 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
Gaia DR3 3344609716230257920,2461128.6232,13.95,0.05,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 3344609716230257920 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:11.26 +14:06:20.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.96 06:08:55.85 +17:07:40.2
192.89951 -1.29242 galactic Ori Second-epoch detections are separated by 4.7" and 2.5 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 29.1232* 06 08 55.85 +17 07 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 J092.2210+17.1268,2461128.6232,13.96,0.05,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
ATO J092.2210+17.1268 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:55.85 +17:07:40.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 01 32.33 +14 49 01.0 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 3345459260761341056,2461128.6232,13.98,0.05,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
Gaia DR3 3345459260761341056 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:32.33 +14:49:01.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.93 06:15:38.04 +17:53:12.8
193.00151 0.47388 galactic Ori Second-epoch detections are separated by 4.1" and 2.5 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 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 29.1232* 06 15 38.04 +17 53 12.8 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 3370369349523493248,2461128.6232,13.93,0.05,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
Gaia DR3 3370369349523493248 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:38.04 +17:53:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.11 05:58:07.88 +17:09:02.1
191.61266 -3.52935 galactic Ori Second-epoch detections are separated by 3.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.5251+17.1516 | 05:58:07.88 +17:09:02.1 (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 29.1232* 05 58 07.88 +17 09 02.1 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
ATO J089.5251+17.1516,2461128.6232,14.11,0.05,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
ATO J089.5251+17.1516 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:07.88 +17:09:02.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.98 06:10:40.74 +15:14:02.4
194.76127 -1.83943 galactic Ori Second-epoch detections are separated by 2.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.6774+15.2319 | 06:10:41.96 +15:14:09.2 (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 29.1232* 06 10 40.74 +15 14 02.4 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
ATO J092.6774+15.2319,2461128.6232,13.98,0.05,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 J092.6774+15.2319 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:40.74 +15:14:02.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.99 06:25:33.70 +17:35:15.0
194.37922 2.41837 galactic Gem Second-epoch detections are separated by 1.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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+17.5919,2461128.6232,13.99,0.05,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
ATO J096.3847+17.5919 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:33.70 +17:35:15.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 01 19.57 +15 34 36.3 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
ASASSN-V J060119.50+153429.8,2461128.6232,14.04,0.05,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
ASASSN-V J060119.50+153429.8 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:19.57 +15:34:36.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 12 51.31 +13 17 02.7 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 3344149020858876288,2461128.6232,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3344149020858876288 20260329.1232 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:51.31 +13:17:02.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.87 06:39:17.07 +15:47:13.6
197.49270 4.51170 galactic Gem Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3358560663362092672 | 06:39:18.40 +15:46:38.7 (Gaia DR3) | RS (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3358560663362092672,2461128.6232,13.87,0.05,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 3358560663362092672 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:39:17.07 +15:47:13.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 52 24.03 +13 07 42.6 14.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.6232,14.09,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:24.03 +13:07:42.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.89 06:36:16.00 +17:59:28.7
195.19303 4.86728 galactic Gem Second-epoch detections are separated by 2.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:36:16.00 +17:59:28.7 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.554+/-0.160 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461128.6232,13.89,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:16.00 +17:59:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.02 06:20:14.51 +13:20:23.6
197.53101 -0.70497 galactic Ori Second-epoch detections are separated by 2.3" and 2.9 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 | 06:20:14.51 +13:20:23.6 (user input) | T | P | (position from user input) 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 29.1232* 06 20 14.51 +13 20 23.6 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,2461128.6232,14.02,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:14.51 +13:20:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 13.96 06:13:50.87 +14:44:31.4
195.56039 -1.40407 galactic Ori Second-epoch detections are separated by 2.6" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 13 50.87 +14 44 31.4 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 3344880917645606144,2461128.6232,13.96,0.05,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 3344880917645606144 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:50.87 +14:44:31.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 16 27.29 +14 57 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,2461128.6232,13.93,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:27.29 +14:57:43.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 49 53.48 +12 29 46.2 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,2461128.6232,14.10,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:53.48 +12:29:46.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.13 06:06:01.07 +16:53:34.0
192.76654 -2.01529 galactic Ori Second-epoch detections are separated by 4.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 06 01.07 +16 53 34.0 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 3349222408025645184,2461128.6232,14.13,0.05,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 3349222408025645184 20260329.1232 14.13CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:01.07 +16:53:34.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.15 06:14:07.62 +18:00:35.3
192.72240 0.21762 galactic Ori Second-epoch detections are separated by 2.4" and 2.9 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 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 29.1232* 06 14 07.62 +18 00 35.3 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 3373364999016141568,2461128.6232,14.15,0.05,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 3373364999016141568 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:07.62 +18:00:35.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 15 51.77 +13 13 57.6 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
target,2461128.6232,14.14,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:51.77 +13:13:57.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.11 06:04:27.92 +16:29:13.6
192.93913 -2.53782 galactic Ori Second-epoch detections are separated by 2.1" and 2.9 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 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 29.1232* 06 04 27.92 +16 29 13.6 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
ATO J091.1205+16.4924,2461128.6232,14.11,0.05,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
ATO J091.1205+16.4924 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:27.92 +16:29:13.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 52 31.28 +12 19 33.1 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,2461128.6232,14.01,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:31.28 +12:19:33.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.02 05:55:56.68 +14:38:13.5
193.53764 -5.23535 galactic Ori Second-epoch detections are separated by 3.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 05 55 56.68 +14 38 13.5 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 3346978682752384256,2461128.6232,14.02,0.05,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 3346978682752384256 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:56.68 +14:38:13.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.21 06:10:29.67 +16:02:29.5
194.03195 -1.48925 galactic Ori Second-epoch detections are separated by 2.3" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3346057979202624768 | 06:10:32.28 +16:02:07.5 (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 29.1232* 06 10 29.67 +16 02 29.5 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 3346057979202624768,2461128.6232,14.21,0.05,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 3346057979202624768 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:29.67 +16:02:29.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 50 03.82 +10 24 32.0 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 3336673681818468096,2461128.6232,13.96,0.05,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 3336673681818468096 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:03.82 +10:24:32.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 17 27.92 +11 05 42.8 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
VARIABLE_NAME,2461128.6232,13.93,0.05,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
VARIABLE_NAME 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:27.92 +11:05:42.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.02 06:10:25.17 +16:38:52.0
193.49202 -1.21266 galactic Ori Second-epoch detections are separated by 3.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.6009+16.6519 | 06:10:25.17 +16:38:52.0 (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 29.1232* 06 10 25.17 +16 38 52.0 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
ATO J092.6009+16.6519,2461128.6232,14.02,0.05,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 J092.6009+16.6519 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:25.17 +16:38:52.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.10 06:20:25.62 +16:52:34.9
194.43335 1.00205 galactic Ori Second-epoch detections are separated by 2.5" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3370012759862921600 | 06:20:27.08 +16:52:11.8 (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 29.1232* 06 20 25.62 +16 52 34.9 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
Gaia DR3 3370012759862921600,2461128.6232,14.10,0.05,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
Gaia DR3 3370012759862921600 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:25.62 +16:52:34.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.15 05:58:52.31 +13:37:23.5
194.77491 -5.12057 galactic Ori Second-epoch detections are separated by 4.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:58:52.31 +13:37:23.5 (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 29.1232* 05 58 52.31 +13 37 23.5 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,2461128.6232,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:52.31 +13:37:23.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.03 06:25:04.28 +16:36:40.6
195.18900 1.85987 galactic Ori Second-epoch detections are separated by 1.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 25 04.28 +16 36 40.6 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 J096.2712+16.6032,2461128.6232,14.03,0.05,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 J096.2712+16.6032 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:04.28 +16:36:40.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 49 46.29 +14 47 43.5 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 3347876021679565184,2461128.6232,14.34,0.05,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 3347876021679565184 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:46.29 +14:47:43.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.10 06:07:09.47 +16:42:47.4
193.05641 -1.86441 galactic Ori Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 07 09.47 +16 42 47.4 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
ATO J091.7968+16.7013,2461128.6232,14.10,0.05,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 J091.7968+16.7013 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:09.47 +16:42:47.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.41 05:58:56.45 +18:06:46.5
190.87229 -2.88370 galactic Ori Second-epoch detections are separated by 3.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:58:56.45 +18:06:46.5 (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 29.1232* 05 58 56.45 +18 06 46.5 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,2461128.6232,14.41,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:56.45 +18:06:46.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 59 52.66 +12 19 21.9 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 3343380324792165120,2461128.6232,14.21,0.05,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 3343380324792165120 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:52.66 +12:19:21.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.09 06:06:04.83 +13:40:16.8
195.59177 -3.56946 galactic Ori Second-epoch detections are separated by 1.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.5163+13.6776 | 06:06:02.93 +13:40:30.4 (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 29.1232* 06 06 04.83 +13 40 16.8 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 J091.5163+13.6776,2461128.6232,14.09,0.05,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
ATO J091.5163+13.6776 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:04.83 +13:40:16.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.32 06:11:18.41 +14:47:53.9
195.21640 -1.91617 galactic Ori Second-epoch detections are separated by 4.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.8379+14.7962 | 06:11:20.29 +14:47:43.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9 1959ApJS....4...23M LF 8 +14 82
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 11 18.41 +14 47 53.9 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
ATO J092.8379+14.7962,2461128.6232,14.32,0.05,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
ATO J092.8379+14.7962 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:18.41 +14:47:53.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.26 05:56:54.46 +15:03:06.2
193.29249 -4.82737 galactic Ori Second-epoch detections are separated by 1.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.2268+15.0496 | 05:56:54.83 +15:03:28.9 (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 29.1232* 05 56 54.46 +15 03 06.2 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 J089.2268+15.0496,2461128.6232,14.26,0.05,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
ATO J089.2268+15.0496 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:54.46 +15:03:06.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.13 06:27:52.40 +16:41:35.9
195.42857 2.49218 galactic Gem Second-epoch detections are separated by 2.7" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3369382709637642240 | 06:27:51.19 +16:42:03.6 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3369382709637642240,2461128.6232,14.13,0.05,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 3369382709637642240 20260329.1232 14.13CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:52.40 +16:41:35.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 3356819105663541632,2461128.6232,14.13,0.05,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 3356819105663541632 20260329.1232 14.13CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:51.85 +15:01:10.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.16 05:58:27.90 +15:59:40.8
192.65804 -4.03381 galactic Ori Second-epoch detections are separated by 1.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 05 58 27.90 +15 59 40.8 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 3348824934574492416,2461128.6232,14.16,0.05,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 3348824934574492416 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:27.90 +15:59:40.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 48 20.40 +13 06 39.3 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
target,2461128.6232,14.44,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:20.40 +13:06:39.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.20 06:10:34.15 +18:09:01.8
192.19283 -0.45640 galactic Ori Second-epoch detections are separated by 5.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3373523298627558400 | 06:10:31.30 +18:08:49.5 (Gaia DR3) | T | P | 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 29.1232* 06 10 34.15 +18 09 01.8 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 3373523298627558400,2461128.6232,14.20,0.05,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 3373523298627558400 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:34.15 +18:09:01.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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,2461128.6232,14.04,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:38:54.23 +17:47:26.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.29 06:27:31.24 +15:16:12.7
196.65073 1.75677 galactic Gem Second-epoch detections are separated by 4.4" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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+15.2532,2461128.6232,14.29,0.05,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
ATO J096.8852+15.2532 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:31.24 +15:16:12.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.39 05:52:03.71 +15:17:56.9
192.49072 -5.71668 galactic Tau Second-epoch detections are separated by 1.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 05 52 03.71 +15 17 56.9 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
Gaia DR3 3348008130574331904,2461128.6232,14.39,0.05,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 3348008130574331904 20260329.1232 14.39CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:03.71 +15:17:56.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.40 05:49:09.18 +15:28:21.4
191.98457 -6.23464 galactic Tau Second-epoch detections are separated by 3.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J087.2916+15.4668 | 05:49:09.18 +15:28:21.4 (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 29.1232* 05 49 09.18 +15 28 21.4 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 J087.2916+15.4668,2461128.6232,14.40,0.05,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
ATO J087.2916+15.4668 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:09.18 +15:28:21.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 11 39.60 +16 27 38.5 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
Gaia DR3 3346141778306377216,2461128.6232,14.38,0.05,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 3346141778306377216 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:39.60 +16:27:38.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.21 05:58:55.65 +14:23:33.8
194.10969 -4.72930 galactic Ori Second-epoch detections are separated by 3.3" and 2.9 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 3346926589089719808 | 05:58:56.38 +14:24:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1931AnHar.100...61C HD 249922
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 58 55.65 +14 23 33.8 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 3346926589089719808,2461128.6232,14.21,0.05,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 3346926589089719808 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:55.65 +14:23:33.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.31 06:19:36.65 +17:40:28.7
193.63739 1.20673 galactic Ori Second-epoch detections are separated by 1.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 19 36.65 +17 40 28.7 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 3370664499677963520,2461128.6232,14.31,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:36.65 +17:40:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 10 28.05 +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+134954.2,2461128.6232,14.09,0.05,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
ASASSN-V J061028.07+134954.2 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:28.05 +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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.28 05:55:50.17 +17:41:15.7
190.87257 -3.73596 galactic Ori Second-epoch detections are separated by 4.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:55:50.17 +17:41:15.7 (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 29.1232* 05 55 50.17 +17 41 15.7 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,2461128.6232,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 14.28CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:50.17 +17:41:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.26 05:49:45.62 +14:44:54.6
192.68782 -6.47404 galactic Tau Second-epoch detections are separated by 3.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J087.4389+14.7468 | 05:49:45.62 +14:44:54.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 49 45.62 +14 44 54.6 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.4389+14.7468,2461128.6232,14.26,0.05,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
ATO J087.4389+14.7468 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:45.62 +14:44:54.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 57 35.77 +15 03 49.6 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,2461128.6232,14.41,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:35.77 +15:03:49.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.27 05:59:50.35 +16:54:20.2
192.02860 -3.29637 galactic Ori Second-epoch detections are separated by 3.1" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 05 59 50.35 +16 54 20.2 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
Gaia DR3 3348989066746631552,2461128.6232,14.27,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:50.35 +16:54:20.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.31 05:58:04.82 +13:32:09.6
194.75584 -5.33090 galactic Ori Second-epoch detections are separated by 3.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3343758896090086400 | 05:58:02.45 +13:31:39.7 (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 29.1232* 05 58 04.82 +13 32 09.6 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
Large-amplitude variable Gaia DR2 3343758896090086400,2461128.6232,14.31,0.05,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
Large-amplitude variable Gaia DR2 3343758896090086400 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:04.82 +13:32:09.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 57 41.34 +17 40 40.5 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,2461128.6232,14.40,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:41.34 +17:40:40.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.28 06:01:56.65 +16:44:38.7
192.41827 -2.93800 galactic Ori Second-epoch detections are separated by 3.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.4905+16.7442 | 06:01:56.65 +16:44:38.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=3.075+/- (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 29.1232* 06 01 56.65 +16 44 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
ATO J090.4905+16.7442,2461128.6232,14.28,0.05,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
ATO J090.4905+16.7442 20260329.1232 14.28CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:56.65 +16:44:38.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.39 05:50:36.42 +14:31:42.7
192.98288 -6.40794 galactic Tau Second-epoch detections are separated by 5.1" and 2.4 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 J087.6514+14.5329 | 05:50:36.42 +14:31:42.7 (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 29.1232* 05 50 36.42 +14 31 42.7 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
ATO J087.6514+14.5329,2461128.6232,14.39,0.05,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
ATO J087.6514+14.5329 20260329.1232 14.39CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:36.42 +14:31:42.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 00 53.07 +12 13 41.6 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
target,2461128.6232,14.20,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:53.07 +12:13:41.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.17 06:06:05.08 +13:21:02.4
195.87321 -3.72417 galactic Ori Second-epoch detections are separated by 1.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 29.1232* 06 06 05.08 +13 21 02.4 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 3344300336848200576,2461128.6232,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3344300336848200576 20260329.1232 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q2b1x1_2026-02-21_21-01-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:05.08 +13:21:02.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.38 06:00:38.99 +15:55:36.4
192.97741 -3.61090 galactic Ori Second-epoch detections are separated by 3.3" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3348858568458675072 | 06:00:39.09 +15:56:15.2 (Gaia DR3) | T | P | 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 29.1232* 06 00 38.99 +15 55 36.4 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
Gaia DR3 3348858568458675072,2461128.6232,14.38,0.05,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 3348858568458675072 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:38.99 +15:55:36.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 56 38.86 +17 44 21.4 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,2461128.6232,14.44,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:38.86 +17:44:21.4 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.38 06:19:59.31 +17:10:05.9
194.12642 1.04726 galactic Ori Second-epoch detections are separated by 3.1" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 29.1232* 06 19 59.31 +17 10 05.9 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 J094.9970+17.1664,2461128.6232,14.38,0.05,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 J094.9970+17.1664 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:19:59.31 +17:10:05.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.48 05:54:24.85 +15:55:48.1
192.22780 -4.91028 galactic Ori Second-epoch detections are separated by 2.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.5942+15.9276 | 05:54:24.85 +15:55:48.1 (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 29.1232* 05 54 24.85 +15 55 48.1 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 J088.5942+15.9276,2461128.6232,14.48,0.05,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
ATO J088.5942+15.9276 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:24.85 +15:55:48.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.32 05:56:30.45 +15:24:06.3
192.93955 -4.73717 galactic Ori Second-epoch detections are separated by 1.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.1277+15.3906 | 05:56:30.06 +15:23:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 56 30.45 +15 24 06.3 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 J089.1277+15.3906,2461128.6232,14.32,0.05,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
ATO J089.1277+15.3906 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:30.45 +15:24:06.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.39 05:58:28.09 +17:33:01.5
191.30514 -3.26085 galactic Ori Second-epoch detections are separated by 3.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.6230+17.5404 | 05:58:28.09 +17:33:01.5 (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 29.1232* 05 58 28.09 +17 33 01.5 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
ATO J089.6230+17.5404,2461128.6232,14.39,0.05,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
ATO J089.6230+17.5404 20260329.1232 14.39CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:28.09 +17:33:01.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.49 05:53:45.27 +15:46:35.8
192.28135 -5.12443 galactic Ori Second-epoch detections are separated by 2.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3348055512654592768 | 05:53:43.55 +15:46:57.1 (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 29.1232* 05 53 45.27 +15 46 35.8 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 3348055512654592768,2461128.6232,14.49,0.05,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
Gaia DR3 3348055512654592768 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:45.27 +15:46:35.8 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.34 06:00:54.64 +15:22:19.2
193.49219 -3.82963 galactic Ori Second-epoch detections are separated by 2.8" and 2.9 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 J090.2227+15.3613 | 06:00:53.46 +15:21:41.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 29.1232* 06 00 54.64 +15 22 19.2 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 J090.2227+15.3613,2461128.6232,14.34,0.05,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
ATO J090.2227+15.3613 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:54.64 +15:22:19.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.20 06:15:24.32 +13:24:20.3
196.91559 -1.70973 galactic Ori Second-epoch detections are separated by 3.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3344130157362715904 | 06:15:25.94 +13:23:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1959ApJS....4...23M LF 8 +13 180
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 15 24.32 +13 24 20.3 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 3344130157362715904,2461128.6232,14.20,0.05,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 3344130157362715904 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:24.32 +13:24:20.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.36 05:59:39.43 +13:09:23.1
195.27728 -5.18400 galactic Ori Second-epoch detections are separated by 2.4" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:59:39.43 +13:09:23.1 (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 29.1232* 05 59 39.43 +13 09 23.1 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
target,2461128.6232,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:39.43 +13:09:23.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.34 06:01:32.19 +16:40:16.4
192.43364 -3.05884 galactic Ori Second-epoch detections are separated by 4.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.3722+16.6657 | 06:01:29.35 +16:39:56.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 01 32.19 +16 40 16.4 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
ATO J090.3722+16.6657,2461128.6232,14.34,0.05,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
ATO J090.3722+16.6657 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:32.19 +16:40:16.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.47 06:10:33.47 +16:28:35.0
193.65819 -1.26628 galactic Ori Second-epoch detections are separated by 1.0" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3346121716516824320 | 06:10:30.66 +16:28:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 10 33.47 +16 28 35.0 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 3346121716516824320,2461128.6232,14.47,0.05,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
Gaia DR3 3346121716516824320 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:33.47 +16:28:35.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.45 05:48:48.99 +15:03:36.3
192.30125 -6.51341 galactic Tau Second-epoch detections are separated by 4.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:48:48.99 +15:03:36.3 (user input) | T | P | (position from user input) J-Ks=0.544+/-0.139 (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 29.1232* 05 48 48.99 +15 03 36.3 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
target,2461128.6232,14.45,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:48.99 +15:03:36.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.45 05:56:31.53 +16:33:11.6
191.94017 -4.15997 galactic Ori Second-epoch detections are separated by 1.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.1382+16.5632 | 05:56:33.14 +16:33:32.3 (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 29.1232* 05 56 31.53 +16 33 11.6 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
ATO J089.1382+16.5632,2461128.6232,14.45,0.05,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 J089.1382+16.5632 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:31.53 +16:33:11.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 06 02 07.05 +16 19 41.2 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,2461128.6232,14.57,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:07.05 +16:19:41.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.30 06:08:01.86 +15:33:58.0
194.16178 -2.23782 galactic Ori Second-epoch detections are separated by 2.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3345925110094675072 | 06:08:01.05 +15:33:25.7 (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 29.1232* 06 08 01.86 +15 33 58.0 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 3345925110094675072,2461128.6232,14.30,0.05,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 3345925110094675072 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:01.86 +15:33:58.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 50 06.04 +12 53 14.1 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 3346244415142170112,2461128.6232,14.38,0.05,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 3346244415142170112 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:06.04 +12:53:14.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.45 05:52:28.71 +14:24:30.1
193.31619 -6.07643 galactic Tau Second-epoch detections are separated by 2.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3347072690997238528 | 05:52:27.08 +14:24:59.9 (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 29.1232* 05 52 28.71 +14 24 30.1 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 3347072690997238528,2461128.6232,14.45,0.05,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 3347072690997238528 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:28.71 +14:24:30.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.41 06:01:17.11 +15:30:04.1
193.42405 -3.68751 galactic Ori Second-epoch detections are separated by 3.1" and 2.9 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 3348638979669417856 | 06:01:14.95 +15:30:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 01 17.11 +15 30 04.1 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
Gaia DR3 3348638979669417856,2461128.6232,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3348638979669417856 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:17.11 +15:30:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.37 05:55:42.04 +14:41:21.9
193.46257 -5.26052 galactic Ori Second-epoch detections are separated by 2.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:55:42.04 +14:41:21.9 (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 29.1232* 05 55 42.04 +14 41 21.9 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
target,2461128.6232,14.37,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:42.04 +14:41:21.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 58 42.60 +11 51 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
VARIABLE_NAME,2461128.6232,14.41,0.05,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
VARIABLE_NAME 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:42.60 +11:51:00.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 58 09.45 +17 20 40.6 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,2461128.6232,14.34,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:09.45 +17:20:40.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.45 06:02:05.99 +16:03:13.3
193.03863 -3.24510 galactic Ori Second-epoch detections are separated by 4.0" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.5152+16.0571 | 06:02:05.99 +16:03:13.3 (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 29.1232* 06 02 05.99 +16 03 13.3 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 J090.5152+16.0571,2461128.6232,14.45,0.05,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 J090.5152+16.0571 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:05.99 +16:03:13.3 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.49 06:10:07.81 +15:00:28.2
194.89571 -2.06447 galactic Ori Second-epoch detections are separated by 3.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.5281+14.9965 | 06:10:07.17 +14:59:54.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE 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 29.1232* 06 10 07.81 +15 00 28.2 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 J092.5281+14.9965,2461128.6232,14.49,0.05,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 J092.5281+14.9965 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:07.81 +15:00:28.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.37 05:52:47.63 +15:52:24.7
192.08077 -5.27569 galactic Tau Second-epoch detections are separated by 2.2" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:52:47.63 +15:52:24.7 (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 29.1232* 05 52 47.63 +15 52 24.7 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
target,2461128.6232,14.37,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:47.63 +15:52:24.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 53 45.05 +15 09 38.0 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,2461128.6232,14.51,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:45.05 +15:09:38.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 53 06.34 +14 57 36.0 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
target,2461128.6232,14.46,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:06.34 +14:57:36.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.34 05:51:06.34 +15:03:05.9
192.58915 -6.04055 galactic Tau Second-epoch detections are separated by 5.4" and 2.4 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 | 05:51:06.34 +15:03:05.9 (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 29.1232* 05 51 06.34 +15 03 05.9 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.7706+15.0575,2461128.6232,14.34,0.05,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
ATO J087.7706+15.0575 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:06.34 +15:03:05.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.69 05:51:24.40 +15:08:08.5
192.55287 -5.93547 galactic Tau Second-epoch detections are separated by 4.0" and 2.9 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 | 05:51:24.40 +15:08:08.5 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 05 51 24.40 +15 08 08.5 14.7 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,2461128.6232,14.69,0.05,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 20260329.1232 14.69CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:24.40 +15:08:08.5 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 54 14.08 +15 13 42.7 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
ZTF J055413.76+151327.0,2461128.6232,14.35,0.05,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
ZTF J055413.76+151327.0 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:14.08 +15:13:42.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.49 06:04:04.16 +17:40:32.2
191.85567 -2.03835 galactic Ori Second-epoch detections are separated by 1.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:04:04.16 +17:40:32.2 (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 29.1232* 06 04 04.16 +17 40 32.2 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,2461128.6232,14.49,0.05,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 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:04:04.16 +17:40:32.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.43 06:20:00.56 +17:12:18.2
194.09636 1.06898 galactic Ori Second-epoch detections are separated by 3.3" and 2.9 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 3370072099128358656 | 06:19:58.50 +17:12:18.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1232* 06 20 00.56 +17 12 18.2 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 3370072099128358656,2461128.6232,14.43,0.05,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
Gaia DR3 3370072099128358656 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:00.56 +17:12:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.46 05:57:32.63 +14:41:17.1
193.68590 -4.87426 galactic Ori Second-epoch detections are separated by 2.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3346988028601435136 | 05:57:30.93 +14:40:58.9 (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 29.1232* 05 57 32.63 +14 41 17.1 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 3346988028601435136,2461128.6232,14.46,0.05,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
Gaia DR3 3346988028601435136 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:32.63 +14:41:17.1 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 54 08.57 +14 53 55.7 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,2461128.6232,14.46,0.05,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
target 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:08.57 +14:53:55.7 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 57 11.85 +14 38 51.9 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,2461128.6232,14.50,0.05,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
target 20260329.1232 14.50CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:11.85 +14:38:51.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.40 06:02:12.90 +14:59:52.0
193.97381 -3.73948 galactic Ori Second-epoch detections are separated by 4.6" and 2.9 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 3348471128050154496 | 06:02:11.23 +15:00:20.6 (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 29.1232* 06 02 12.90 +14 59 52.0 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
Gaia DR3 3348471128050154496,2461128.6232,14.40,0.05,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
Gaia DR3 3348471128050154496 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:12.90 +14:59:52.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.55 06:06:52.06 +15:48:39.0
193.81164 -2.36387 galactic Ori Second-epoch detections are separated by 5.9" and 2.5 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 J091.7203+15.8042 | 06:06:52.06 +15:48:39.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A0III (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 29.1232* 06 06 52.06 +15 48 39.0 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
ATO J091.7203+15.8042,2461128.6232,14.55,0.05,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 J091.7203+15.8042 20260329.1232 14.55CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:06:52.06 +15:48:39.0 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.50 05:56:30.91 +12:09:19.9
195.77361 -6.34387 galactic Ori Second-epoch detections are separated by 1.9" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3343025453116714624 | 05:56:28.93 +12:09:28.4 (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 29.1232* 05 56 30.91 +12 09 19.9 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
Gaia DR3 3343025453116714624,2461128.6232,14.50,0.05,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 3343025453116714624 20260329.1232 14.50CV 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:30.91 +12:09:19.9 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1232 2461128.6232 14.47 06:03:42.69 +13:07:00.2
195.79668 -4.34260 galactic Ori Second-epoch detections are separated by 2.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.9253+13.1153 | 06:03:42.69 +13:07:00.2 (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 29.1232* 06 03 42.69 +13 07 00.2 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 J090.9253+13.1153,2461128.6232,14.47,0.05,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
ATO J090.9253+13.1153 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:42.69 +13:07:00.2 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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 29.1232* 05 58 23.77 +11 50 43.6 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
VARIABLE_NAME,2461128.6232,13.72,0.05,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
VARIABLE_NAME 20260329.1232 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:23.77 +11:50:43.6 ;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_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q2b1x1_2026-02-21_21-01-32_20_00sec_-14_90C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20_00sec_-15_00C_LIGHT_0059_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: 2461128.62345213 29.03.2026 02:57:36.264 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
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: 8 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): 27083
Objects passed selection criteria: 26987
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: 21043.8
Average stars matched: 20505.8 (97.4434 %)
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 22:36:43 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: 2461128.62345213 29.03.2026 02:57:36.264 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1393
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: 72 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): 156307
Objects passed selection criteria: 156021
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: 138405
Average stars matched: 132872 (96.0023 %)
Memory usage VmPeak: 2634872 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 22:39:16 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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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: 2461128.62294015
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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits exists and is non-empty
Saving wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits'
wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits exists and is non-empty
Saving wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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 06:13:26.063 +14:01:28.81
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 06:13:26.408 +14:01:45.29
Angular distance between the image centers 0.12 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 06:13:26.063 +14:01:28.81
Second-epoch second image center 06:13:26.408 +14:01:45.29
Angular distance between the image centers 0.00479 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.7edcBqU6DK
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.Jw9Cf5XfMp
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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits &> /tmp/tmp.2eEpCUhUsF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits &> /tmp/tmp.IrqoEcKxPA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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 16 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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
2.3 pix fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
14.4 mag. fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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.7edcBqU6DK (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_223337_TTUQ2b1x1_704_qspcU5Q4/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.Jw9Cf5XfMp (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_223337_TTUQ2b1x1_704_qspcU5Q4/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.2eEpCUhUsF (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_223337_TTUQ2b1x1_704_qspcU5Q4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1508, passed=16423
Got 16423 stars (including 14898 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 16423 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 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: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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: 0.63"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 913 stars left (next iteration limit 1002)
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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits -region wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IrqoEcKxPA (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_223337_TTUQ2b1x1_704_qspcU5Q4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1556, passed=16258
Got 16258 stars (including 14680 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat
util/solve_plate_with_UCAC5 got 16258 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 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 911 stars left (next iteration limit 999)
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_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits -region wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/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_223337_TTUQ2b1x1_704_qspcU5Q4/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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits'
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits'
Preparing the HTML report for the field Ori-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51575.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__out51580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52060.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out51987.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 51569_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51569_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:31.15 +12:14:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 3.430 3331943097461376640 093.38023444500 +12.24767894902 11.4174 10.4847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51573_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51573_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:41.68 +16:32:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 2.594 3369541211110732672 096.42382454315 +16.54082334187 10.9869 10.2679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51575_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51575_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:25.66 +16:03:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 3.480 3357845053090488832 100.35714121559 +16.06408544540 11.0387 10.6139 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 51576_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51576_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:53.70 +14:54:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 3.160 3356239285078194176 099.47425692088 +14.91568822201 10.8651 10.0886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.160#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51578_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:26.90 +17:16:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 2.845 3349986323792979328 088.86212951416 +17.27215543188 11.0935 10.8277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51580_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51580_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:18.75 +14:00:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.02, MAG_FAINT_SEARCH_LIMIT=10.00)GAIADR2_OUTPUT=# 2.130 3345194347178716800 092.07770715289 +14.00376444567 8.3071 7.1898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51673_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51673_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:18.79 +13:59:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.14, MAG_FAINT_SEARCH_LIMIT=11.12)GAIADR2_OUTPUT=# 3.121 3345194347176271872 092.07802470555 +13.98856167066 10.5449 10.4762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51682_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51682_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:15.42 +15:33:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 2.660 3345750115942949120 092.81452392098 +15.56272641147 10.3958 9.9883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51718_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51718_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:25.25 +15:43:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.50, MAG_FAINT_SEARCH_LIMIT=11.48)GAIADR2_OUTPUT=# 1.336 3357096216952323968 098.85533171442 +15.71842612673 10.4561 9.7252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51760_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51760_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:05.10 +15:12:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 3.364 3348478657131124480 090.52162924754 +15.19941809654 10.6687 9.8662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51846_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51846_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:59.94 +18:04:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 3.232 3350286009430416896 090.75017501953 +18.06644822458 11.2410 11.0507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51856_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51856_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:52.07 +14:13:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51875_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51875_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:44.04 +16:56:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 2.386 3349354791800163072 090.43370513177 +16.93625582270 11.1866 10.4013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51945_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 51945_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:43.84 +16:47:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 2.640 3369392296004628736 096.93299990475 +16.78342297646 10.8171 9.7201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51987_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 51987_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 52060_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 52060_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:01.67 +10:51:32.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)
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 ####
06:35:44.94 +11:17:01.3
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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits exists and is non-empty
wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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 06:13:26.063 +14:01:28.81
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 06:13:26.408 +14:01:45.29
Angular distance between the image centers 0.12 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 06:13:26.063 +14:01:28.81
Second-epoch second image center 06:13:26.408 +14:01:45.29
Angular distance between the image centers 0.00479 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.YEDtmKTHii
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.gxYSgX2Ije
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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits &> /tmp/tmp.d4beS4osjb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits &> /tmp/tmp.wHVPrlpK6U
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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 1079 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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
2.1 pix fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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
14.5 mag. fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
14.6 mag. fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
All-image limiting magnitude estimate: 14.5 (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.YEDtmKTHii (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_223337_TTUQ2b1x1_704_qspcU5Q4/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.gxYSgX2Ije (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_223337_TTUQ2b1x1_704_qspcU5Q4/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.d4beS4osjb (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_223337_TTUQ2b1x1_704_qspcU5Q4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=12458, passed=128427
Got 128427 stars (including 115809 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 128427 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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 910 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: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 906 stars left (next iteration limit 994)
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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits -region wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.wHVPrlpK6U (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_223337_TTUQ2b1x1_704_qspcU5Q4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
Checking if the catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat corresponding to the image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits
WCS catalog name: wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=12485, passed=130078
Got 130078 stars (including 117422 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat
util/solve_plate_with_UCAC5 got 130078 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 902 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: 0.64"
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 901 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: 0.78"
Excluding outliers - 898 stars left (next iteration limit 985)
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_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits -region wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/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_223337_TTUQ2b1x1_704_qspcU5Q4/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_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Ori-02-Q2b1x1_223337_TTUQ2b1x1_704_qspcU5Q4/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-56-52_20.00sec_-15.00C_LIGHT_0059.fits
Saving fully-calibrated image wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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_223337_TTUQ2b1x1_704_qspcU5Q4/wcs_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060.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
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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__out200056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200138.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200228.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200230.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200365.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200430.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200466.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200514.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200579.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200599.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200606.dat to exclusion_list_gaiadr2.txt
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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__out200615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200631.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200640.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200651.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out200657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200675.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__out200683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200726.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__out200731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200732.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__out200737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200760.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__out200766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200778.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__out200783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200792.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__out200795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200824.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__out200835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200836.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__out200840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200853.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__out200859.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__out200864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200893.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__out200902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200913.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__out200920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203779.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__out203804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out200033.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200160.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200201.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200239.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200300.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200317.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200357.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200369.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200401.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200404.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200408.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200450.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200477.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200544.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200577.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200613.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200672.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200699.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200702.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200704.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200716.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200738.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200741.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200749.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200802.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200830.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202097.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202137.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202372.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202392.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202505.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202508.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202790.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202793.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202797.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out202973.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203020.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203081.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203111.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203211.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203281.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203294.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203373.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203414.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203565.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203650.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203664.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203778.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203811.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203818.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203932.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203956.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204012.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204013.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204021.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204054.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204113.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204199.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204421.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204576.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204745.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204760.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205210.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205305.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205306.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out205425.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out124797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200048.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__out200070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200446.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__out200463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203144.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203190.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203415.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203649.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203717.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203733.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203819.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203843.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203882.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203921.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203959.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out203969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204066.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204121.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204159.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204186.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204216.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204386.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out204686.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205001.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205167.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205255.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205431.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205499.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__out205527.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out205609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205653.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 496s
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: 231s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200033_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200033_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:23.41 +11:58:01.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200047_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200047_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200048_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200048_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200056_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200056_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:11.62 +13:37:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 5.591 3345084460439206144 091.79804492464 +13.61951732011 14.2478 13.5950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200057_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200057_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200061_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200061_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200068_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200068_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:11.97 +13:48:07.7 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 200070_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200070_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200078_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200078_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:23.51 +15:36:00.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)
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Considering the candidate 200079_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200079_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200085_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200085_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200093_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200093_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:37.62 +15:10:29.3 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 200094_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200094_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200095_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200095_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200102_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200102_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200103_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200103_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200108_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200108_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200111_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200111_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200112_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200112_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200119_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200119_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200127_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200127_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:18:54.69 +15:27:34.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)
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Considering the candidate 200132_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200132_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200133_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200133_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:24:04.46 +16:00:04.3 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 200134_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200134_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200136_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200136_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200138_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200138_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:36.59 +10:34:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 5.554 3329979541493885312 092.65242831194 +10.57231871871 14.3976 14.0038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200141_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200141_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200142_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200142_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:46.64 +14:56:23.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)
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Considering the candidate 200143_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200143_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200144_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200144_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200157_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200157_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200160_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200160_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:28.58 +15:07:57.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)
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Considering the candidate 200161_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200161_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200166_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200166_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:50.05 +14:00:23.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)
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Considering the candidate 200172_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200172_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200175_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200175_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:24:40.28 +16:13:07.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
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Considering the candidate 200176_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200176_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:19.94 +16:00:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 5.709 3348672446054291712 090.33287728651 +15.99928778362 14.2667 13.7508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200177_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200177_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200183_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200183_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:05.62 +11:18:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 5.235 3342311187172762496 091.02375000867 +11.29911075103 14.4490 13.7315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200189_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200189_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200190_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200190_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200191_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200191_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200194_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200194_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200196_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200196_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200200_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200200_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:31:46.48 +18:03:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 5.779 3371266791530693376 097.94389601844 +18.05446502367 14.1973 13.5178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200201_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200201_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:47.24 +15:49:36.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)
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Considering the candidate 200203_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200203_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:03.97 +14:04:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.849 3346887560726999424 089.51701825793 +14.07174834440 14.4755 13.6871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200205_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200205_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:40.25 +12:41:58.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)
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Considering the candidate 200206_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200206_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:23.00 +11:56:36.6 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 200208_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200208_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200209_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200209_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200214_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200214_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200218_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200218_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200219_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200219_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200220_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200220_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200221_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200221_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:44.57 +11:23:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200223_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200223_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200225_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200225_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200226_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200226_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:27.43 +14:56:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 4.998 3347235964178748160 088.11382158097 +14.94685457855 14.2416 13.7626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200227_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200227_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:36.55 +13:06:44.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)
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Considering the candidate 200228_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200228_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:12.38 +13:10:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 5.672 3332331126286336384 095.80177256102 +13.18112975576 13.9658 13.4123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200229_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200229_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:57.89 +15:45:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 5.579 3345803992016144256 093.99095331315 +15.76074756179 14.0875 13.4544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200230_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200230_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:19.47 +16:09:14.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)
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Considering the candidate 200232_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200232_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200235_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200235_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:57.95 +15:01:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 5.788 3344941798804457984 094.24129347272 +15.02623341245 13.9031 13.2621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200236_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200236_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:39.55 +11:18:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 5.784 3336883894697420928 087.91375115223 +11.31162000550 14.4326 13.7305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200237_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200237_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:19.09 +17:04:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 5.728 3349794463311580672 088.82910632706 +17.07429763544 13.7161 12.9004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200239_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200239_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:17.78 +11:39:56.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)
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Considering the candidate 200242_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200242_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:09:10.24 +17:52:00.9 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 200247_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200247_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200249_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200249_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:44.58 +16:25:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 4.030 3369221081427295488 095.68566561585 +16.42443890942 14.6457 14.0352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200253_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200253_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200255_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200255_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:42.07 +13:43:34.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 200256_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200256_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:00.22 +15:47:08.9 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 200259_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200259_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:46.82 +18:07:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 5.480 3371161994327905152 098.69486064103 +18.12510374171 13.8721 13.2739 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 200260_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200260_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200270_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200270_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200272_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200272_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200273_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200273_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 200274_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200274_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:31:14.54 +13:44:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.099 3355599300590144000 097.81052907246 +13.74366794322 13.9161 13.1865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200275_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200275_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:37.98 +11:22:45.4 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 200277_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200277_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200284_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200284_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:06:46.37 +11:27:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 5.817 3342290743128165760 091.69336480523 +11.45466934716 13.8570 13.3539 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 200286_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200286_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200287_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200287_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200288_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200288_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200289_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200289_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200293_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200293_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200295_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200295_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:08.56 +17:03:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 5.441 3350116242261000064 090.03538312384 +17.06512434241 13.6886 13.1673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200296_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200296_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200300_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200300_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:39:36.20 +13:44:49.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 200304_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200304_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200305_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200305_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:48.15 +10:52:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200306_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200306_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200307_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200307_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200308_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200308_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:41.34 +13:39:50.1 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 200309_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200309_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200313_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200313_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200315_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200315_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:39:39.11 +13:10:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 5.835 3352365568175414144 099.91276972888 +13.17744526742 14.1658 13.4295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200317_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200317_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:55.77 +16:31:38.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 200322_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200322_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:49.95 +12:52:23.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 200324_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200324_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200326_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200326_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200331_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200331_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200332_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200332_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:02.40 +15:30:12.4 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 200336_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200336_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:58.78 +14:38:50.8 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 200341_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200341_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:22.43 +14:22:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 5.681 3347071969442763008 088.09315529306 +14.36778278184 13.8632 13.3093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200342_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200342_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:15.53 +17:23:49.5 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 200345_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200345_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:53.09 +11:45:52.0 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 200349_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200349_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:33.80 +13:33:16.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)
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Considering the candidate 200350_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200350_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:33.51 +10:55:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.684 3342060361081894528 089.38942968141 +10.92268268450 13.7346 13.2441 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 200355_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200355_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:05.66 +14:24:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.775 3355963097201792000 100.27322513003 +14.39913649209 13.5856 12.6941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200356_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200356_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:39.13 +17:03:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 5.376 3369492282842716544 097.16279143249 +17.05277609235 13.8832 13.1862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200357_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200357_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:26.24 +14:04:31.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
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Considering the candidate 200358_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200358_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:53.76 +18:03:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 5.747 3369814882130716672 096.97389761946 +18.05035112483 14.0311 13.5459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.747#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200363_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200364_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200364_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:33.65 +11:47:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.748 3330952854101293184 095.88869910125 +11.78600597640 13.5899 12.5014 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 200365_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200365_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:33.32 +12:13:56.9 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 200366_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200366_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200367_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200367_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:22.18 +14:41:38.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 200368_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200368_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200369_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200369_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:27.26 +17:21:41.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
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Considering the candidate 200370_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200370_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200371_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200371_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:56.80 +13:55:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 4.955 3356358101053121920 097.48685176899 +13.92202417135 13.8102 13.2612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200372_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200372_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 200378_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200378_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:52.09 +12:31:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.354 3343298754773067008 088.46736349939 +12.52908209769 14.2720 13.9507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200379_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200379_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200380_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200380_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200382_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200382_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200383_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200383_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200384_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200384_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200385_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200385_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200388_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200388_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:19:59.89 +10:44:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 5.047 3330727110621060992 094.99994275614 +10.73601563726 14.1595 13.8556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200391_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200391_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:15.15 +10:00:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.439 3341699858707442304 090.06280947663 +10.01032693488 13.5676 12.7343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.439#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200395_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:04.09 +14:22:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 4.141 3346911578183730944 089.26730959591 +14.37190717714 14.0834 13.5569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200396_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200396_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200401_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200401_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:45.82 +11:20:48.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 200402_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200402_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:58.66 +10:31:06.8 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 200404_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200404_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:55.24 +14:42:53.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 200406_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200406_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:49.19 +10:35:12.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 200407_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200407_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:04.94 +13:51:50.0 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 200408_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200408_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:28.05 +13:42:36.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 200412_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200412_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200416_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200416_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200418_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200418_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200425_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200425_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200426_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200426_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200429_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200429_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:20.75 +15:59:29.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 200430_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200430_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:57.18 +17:24:05.6 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 200433_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200433_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:14.18 +11:58:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.140 3331301949042868480 096.80918009469 +11.97515872770 13.8314 13.3265 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#
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Considering the candidate 200439_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200439_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:54.60 +16:03:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200441_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200441_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200442_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200442_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200444_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200444_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200445_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200445_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:33:08.50 +16:30:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 5.150 3357404217647409536 098.28528121886 +16.50074210242 13.3486 12.4444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200446_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200446_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200447_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200447_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:48:46.32 +15:33:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 5.636 3347997483354073728 087.19279906293 +15.55408530613 13.6862 13.0663 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200449_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200449_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:05.06 +12:54:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 5.430 3343652591359904512 089.52148175641 +12.90734812780 13.8035 13.2915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200450_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200450_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:27.73 +14:28:12.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200453_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200453_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:07.97 +14:15:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.311 3346860107295167488 088.78399670139 +14.26305030234 13.7315 13.3243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200454_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200454_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200459_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200459_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200461_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200461_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:48.25 +13:57:19.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200463_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200463_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200466_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200466_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:25.61 +17:39:57.3 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 200471_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200471_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200472_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200472_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:55.44 +14:35:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200475_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200475_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200476_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200476_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:31:24.65 +16:39:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.092 3369410437946399488 097.85290745181 +16.66184853411 13.5992 13.0458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200477_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200477_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:43.43 +13:22:51.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200479_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200479_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200481_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200481_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200483_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200483_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:28.53 +11:04:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.352 3342256245951159552 091.11878939836 +11.07804341997 14.0023 13.5613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200484_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200484_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:25.52 +11:51:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.381 3343012847390142720 088.85600951954 +11.86037268727 14.0025 13.5769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200487_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200487_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:16.18 +10:15:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200488_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200488_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200492_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200492_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:09.68 +13:57:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.604 3346833581577034496 088.04044301436 +13.95989233941 13.7688 13.2035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200494_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200494_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:58.31 +12:28:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 4.197 3352264825423369984 100.24295910976 +12.47247298012 13.9232 13.2871 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 200497_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200497_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:38.75 +15:31:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.370 3356298585688310656 099.66139324715 +15.51781526961 13.3108 12.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200498_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200498_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200499_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200499_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200500_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200500_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:02.97 +13:05:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.562 3343356268679297792 088.51253988649 +13.09285235899 13.5524 13.0160 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200503_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200503_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:24.20 +14:54:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.020 3356942800721076096 098.10104980370 +14.90042701750 13.2661 12.2119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200504_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200504_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200505_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200505_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:49.00 +15:14:47.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200506_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200506_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200507_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200507_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:18:32.36 +10:16:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.762 3329207649972301440 094.63519888818 +10.27969049065 13.8487 13.4666 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200508_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200508_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200509_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200509_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:03.08 +17:39:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 5.456 3350036699466846592 089.01264130404 +17.65052338538 13.5511 12.6845 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 200511_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200511_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:31.17 +16:54:09.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200513_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200513_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:19.40 +16:19:07.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200514_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200514_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:47.34 +18:16:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 5.873 3350483135547291648 089.19730882046 +18.28131407127 13.6989 13.1641 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#
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Considering the candidate 200516_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200516_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200517_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200517_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:48:26.85 +11:36:15.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 200518_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200518_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:18:06.76 +11:08:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.785 3331549888915150592 094.52836003891 +11.13587663649 13.5923 13.0904 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 200519_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200519_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:39.45 +17:48:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.444 3371059323133177728 098.66492429238 +17.80980317538 13.5722 12.9626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200521_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200521_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:56.62 +10:40:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.809 3329283859871083520 094.23581392777 +10.67791807562 13.8762 13.4055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200524_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200524_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:29.17 +16:25:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.423 3349695232387854080 089.37129527248 +16.42876648229 13.5147 12.9851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200528_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200528_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:21.95 +16:07:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200533_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200533_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200542_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200542_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:41.24 +11:58:50.8 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 200543_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200543_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200544_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200544_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:59.88 +17:13:50.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 200547_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200547_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:24.81 +14:14:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 5.816 3344642697280983296 095.10301443730 +14.24331170662 13.6468 13.1532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200549_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200549_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200550_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200550_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200551_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200551_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:10.83 +13:44:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.860 3346638727500322304 087.54529630596 +13.74393638368 13.4589 13.0991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200553_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200553_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:51.15 +16:41:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.688 3369382709637645056 096.96340584050 +16.69350357897 13.6449 12.8242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200555_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200555_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:56.71 +17:15:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.791 3369700812095248512 096.73628271865 +17.25403033645 13.3042 12.4104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200558_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200558_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200559_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200559_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:51.08 +18:07:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.452 3371118769777266688 099.21288086775 +18.13048623297 13.3600 12.5998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200561_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200561_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:39:44.85 +13:48:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.177 3355801950028702976 099.93655730155 +13.81106776760 13.4117 12.5942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200563_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200563_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:41.08 +16:47:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 5.564 3370035299851323392 094.42117853251 +16.79106557273 13.5311 12.8922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200564_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200564_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:09.28 +15:02:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.970 3356244920075217408 099.53865588937 +15.04289723954 13.5403 13.0603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200565_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200565_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:05.35 +14:27:04.6 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 200568_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200568_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:33:19.46 +18:04:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.699 3371082382814210944 098.33138212551 +18.06972269078 13.7119 13.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200569_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200569_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200572_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200572_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:24.38 +15:56:58.6 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 200574_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200574_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:16.84 +13:28:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.990 3355437328785134080 099.31988454668 +13.47186350034 13.4147 12.7857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200576_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200576_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:42.47 +18:00:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 5.891 3371111244994678400 098.92729980490 +18.01406271266 13.4307 12.6286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200577_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200577_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:51.21 +17:55:14.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 200578_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200578_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200579_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200579_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:08.20 +13:54:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.061 3346820726737024512 088.53398954816 +13.90621581515 13.5417 13.1090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200582_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200582_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200583_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200583_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:38.20 +17:17:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200584_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200584_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:02.72 +14:48:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.755 3347181160391358336 088.51116686748 +14.80735405641 13.4933 12.7286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200585_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200585_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:51.83 +12:31:31.9 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 200587_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200587_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200593_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200593_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:38.91 +10:09:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200595_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200595_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:55.44 +13:34:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 5.662 3343762233284137984 089.48082259012 +13.56810345886 13.5926 13.3361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200597_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200597_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:36.76 +15:10:26.4 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 200599_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200599_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:09.26 +14:22:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.771 3344800378418959872 093.53848551841 +14.37898613905 14.0608 13.6815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200601_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200601_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200602_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200602_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:47.79 +13:23:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 5.613 3343787006656105344 089.94943995237 +13.38691578193 13.3344 12.4578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200603_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200603_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:58.57 +14:46:34.1 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 200604_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200604_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200605_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200605_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200606_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200606_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:33:14.95 +17:55:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.814 3371071211602935680 098.31183692162 +17.91781816822 13.6330 13.2013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200607_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200607_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200608_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200608_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:50.99 +12:47:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.135 3355326003233356544 099.21253469582 +12.79682615899 13.2400 12.3342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200609_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200609_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:17.45 +09:59:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.800 3341707658367979520 090.32255788627 +09.98884150676 13.5265 13.0828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200611_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200611_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:12.87 +12:50:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.599 3332069923556110976 094.30346753071 +12.84378724923 13.6724 13.1760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200613_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200613_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:44.19 +16:51:54.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 200615_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200615_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:48.61 +15:24:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 5.758 3348016071973828736 088.20309573526 +15.40843691600 13.7605 13.2759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200616_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200616_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200617_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200617_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:08.01 +13:41:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.626 3346452841315535104 087.78306724763 +13.69333373539 13.6435 13.1746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200624_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200624_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200625_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200625_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:28.33 +16:54:52.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 200626_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200626_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:15.71 +09:56:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200628_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200628_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:31:08.68 +12:34:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.691 3331255116718177280 097.78599835561 +12.57137676187 13.3170 12.7319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200631_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200631_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:12.44 +15:20:15.3 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 200633_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200633_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:22.82 +13:03:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 5.586 3346352781462233856 088.34498553294 +13.04872890317 13.3928 12.8155 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#
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Considering the candidate 200638_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200638_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200640_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200640_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:15.52 +15:15:25.7 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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200641_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:23.54 +18:09:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.040 3370577191581233536 096.59810207859 +18.15685003792 13.0528 12.5489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200642_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200642_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:48.29 +17:41:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.729 3371010394864330368 098.70106835079 +17.69799886137 13.4259 12.7890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200646_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200646_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:33:34.36 +17:53:05.1 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 200651_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200651_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:43.11 +10:44:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.702 3330164225086672256 092.17956786094 +10.73652817343 13.1859 12.3657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200652_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200652_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:58.34 +15:26:18.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 200654_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200654_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:28.47 +14:40:23.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 200656_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200656_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:30:13.86 +15:21:58.7 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 200657_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200657_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:02.51 +16:40:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.095 3349705570371528320 089.51066043447 +16.67337576531 13.4444 12.9010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200659_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200659_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:40.55 +15:46:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.511 3348804937206620928 088.91889051539 +15.76760940675 13.3626 12.8941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200660_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200660_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200661_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200661_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:22.46 +14:30:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200662_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200662_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200666_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200666_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200667_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200667_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:09.48 +14:33:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.342 3355980899845317248 100.03927581756 +14.55855973955 13.4192 13.2403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200668_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200668_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:05.55 +15:32:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.150 3347282727777862144 088.77285938371 +15.54000922028 13.2288 12.7103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200669_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200669_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:23.68 +12:57:13.0 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 200670_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200670_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200672_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200672_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:38.93 +15:57:11.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
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Considering the candidate 200675_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200675_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:54.81 +13:07:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.480 3355364554859351680 099.47766021176 +13.12849639098 13.2502 12.7300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200677_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200677_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:14.23 +16:46:07.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 200678_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200678_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:33:38.84 +18:00:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.221 3371078186628115072 098.41154734941 +18.00690866914 13.2750 12.7495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200683_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200683_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:59.11 +14:43:10.5 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 200685_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200685_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:14.88 +15:57:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 5.836 3348867849887081728 089.81213057091 +15.96460605318 13.4483 13.1512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.836#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200688_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:24.50 +14:24:25.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 200689_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200689_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:56.30 +13:42:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.359 3343858131313951872 089.48522629792 +13.69989014071 13.2025 12.7785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200690_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200690_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:56.44 +13:58:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 5.241 3344587927857524736 093.73459045725 +13.97962793871 12.9646 12.1577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200692_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200692_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:21.27 +16:11:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.164 3357369789189778048 098.08839133215 +16.19875414686 13.3304 12.7964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200694_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200694_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:26.32 +12:32:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.940 3355235018645886464 098.60956251724 +12.54490924979 13.0812 12.6075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200698_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200698_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:38.94 +14:24:43.4 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 200699_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200699_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:12.22 +15:29:04.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 200701_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200701_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:24.04 +17:30:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.269 3349489413256128384 091.10006874007 +17.51490052921 13.2829 12.7212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.269#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200702_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:41.99 +15:47:10.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 200704_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200704_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:47.85 +14:01:52.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 200705_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200705_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:30:10.24 +15:59:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 5.751 3357277219757852928 097.54247058600 +15.99344144549 13.1387 12.7613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.751#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200707_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:02.21 +13:08:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200708_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200708_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:44.34 +18:06:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.188 3370517538778148736 095.68467336499 +18.10336616559 13.3287 12.8092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200714_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200714_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200715_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200715_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:33.63 +10:55:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.009 3327790482561445120 099.63954028936 +10.92201786497 13.2051 12.7392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200716_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200716_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:01.53 +14:25:01.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 200717_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200717_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200718_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200718_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200719_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200719_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:11.44 +17:08:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.912 3358906219250904832 099.54767271869 +17.13480225109 13.0151 12.2435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200724_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200724_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:29.88 +14:18:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.888 3347047470948879744 087.87392731378 +14.30660027073 13.0218 12.0957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200725_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200725_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:05.65 +11:35:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 5.124 3342193122814667264 089.77348825008 +11.58321664244 13.2562 12.7805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.124#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200726_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:40.47 +17:48:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.127 3370505650308686848 095.41856366246 +17.79946591961 13.2070 12.6618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200729_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200729_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:25.30 +11:13:42.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 200730_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200730_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:12.92 +14:52:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.134 3356757155055950592 097.05348362975 +14.86908674552 13.0884 12.7563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200731_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200731_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:01.19 +15:56:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.172 3348292908385419392 087.25500421569 +15.94636983274 12.9733 12.4627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200732_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200732_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:26.31 +17:51:36.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)
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Considering the candidate 200733_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200733_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:30.27 +17:05:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.562 3350117994607647616 090.12592322370 +17.08924751434 13.1521 12.5660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.562#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200734_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:36.19 +10:15:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.506 3329935187370341504 092.65063014769 +10.25417316896 13.1642 12.6042 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 200737_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200737_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:41.73 +10:31:26.1 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 200738_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200738_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:48:32.32 +11:28:52.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 200739_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200739_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:53.72 +13:09:12.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 200740_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200740_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:07.67 +13:03:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.851 3332091737690035200 094.03196200172 +13.05398581225 13.0115 12.3067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200741_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200741_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:54.54 +16:12:52.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 200742_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200742_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200743_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200743_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:33.85 +14:06:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.608 3346891443377449216 089.39226500715 +14.11332481626 13.5095 12.9227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200746_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200746_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:39:42.83 +14:46:25.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 200748_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200748_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:30:27.13 +17:19:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.723 3369526535206375808 097.61303605468 +17.32449352883 13.2195 12.9856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200749_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200749_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:49.61 +15:40:49.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 200750_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200750_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:29.89 +16:07:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 5.264 3369142874366218880 095.62489979384 +16.12782876583 13.0531 12.2009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200752_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200752_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:37.69 +15:31:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200753_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200753_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:35.03 +10:51:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.918 3341906601253420160 090.14586844581 +10.85349865892 13.2945 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200755_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200755_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:16.16 +12:18:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.632 3343057682551291776 089.31718168155 +12.31399977869 13.1485 12.5704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200758_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200758_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:32.63 +15:59:28.8 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 200759_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200759_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200760_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200760_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:09.65 +12:06:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.920 3352171981108691328 099.04029753389 +12.10352579703 12.6584 11.7470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200762_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200762_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:03.36 +10:47:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 5.770 3336838711641618944 087.26368309693 +10.79701114344 13.1478 12.6684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.770#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200763_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:28.61 +17:53:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.864 3350416408935551360 089.11880635332 +17.88587086455 12.8342 11.9671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200764_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200764_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:48.83 +14:32:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.495 3356500109852161280 098.20344616657 +14.53708489604 13.3442 12.9376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200766_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200766_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:04.08 +17:33:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.906 3359036477018822400 100.01702250302 +17.55869300511 12.8368 11.9846 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 200770_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200770_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:56.97 +17:17:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.587 3350127718413686400 090.23726801113 +17.28697909644 13.0538 12.5377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.587#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200771_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:47.07 +15:00:21.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 200772_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200772_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:48:21.33 +15:00:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.429 3347943263687112576 087.08858130088 +15.01507435116 12.8047 11.9894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200774_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200774_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 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=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)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 200777_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200777_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:31.84 +17:09:23.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)
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Considering the candidate 200778_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200778_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:40.70 +10:09:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.344 3327646107239611136 098.91946569345 +10.16410450905 13.0310 12.4233 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 200779_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200779_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:26.59 +12:41:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200780_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200780_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:49.17 +14:31:11.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)
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Considering the candidate 200781_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200781_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 200782_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200782_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:39:04.57 +13:02:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.560 3352362613238032896 099.76842513863 +13.03571450182 13.2186 12.8475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200783_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200783_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:10.09 +15:32:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 5.587 3368829376111506304 095.54181194571 +15.54568608354 12.9527 12.4408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200785_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200785_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:06.32 +10:08:48.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 200786_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200786_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:31.44 +13:07:49.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
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Considering the candidate 200787_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200787_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:24.65 +17:04:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.077 3358801628206452736 100.10263151082 +17.07073178886 12.8977 12.3066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.077#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200789_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:53.90 +12:19:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.109 3343380320494676224 089.97466954151 +12.33008326933 13.1537 12.7177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.109#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200792_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:51.24 +12:04:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.645 3342460617674638592 091.96360584871 +12.07349176561 12.9152 12.3905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200793_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200793_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:13.80 +12:38:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.568 3344028280737452160 092.80757431934 +12.64692750551 13.0518 12.5275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.568#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200794_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:02.29 +10:06:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.876 3330465839170971648 095.75901385666 +10.10594864167 12.7586 12.3087 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 200795_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200795_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:18:29.64 +16:11:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 5.451 3369857110247115008 094.62334651220 +16.18493734044 12.9128 12.3724 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 200798_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200798_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:13.72 +14:25:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.125 3356107614262507392 099.05728116838 +14.43141512701 12.9394 12.4287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200802_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200802_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:25.34 +17:42:20.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 200803_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200803_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:56.24 +13:21:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.859 3346416591791870080 087.48443109399 +13.35695909560 12.8991 12.3623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200806_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200806_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:51.96 +15:59:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 5.570 3358580317132401536 099.71605556376 +15.99004067513 12.6742 11.9258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200808_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200808_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:14.06 +13:40:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.164 3355785358575117696 100.05818685553 +13.68218700450 12.6991 12.4615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200812_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200812_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:42.72 +10:29:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200813_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200813_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:18:11.42 +12:49:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.635 3332028588791330688 094.54731863566 +12.82807196706 12.8564 12.5114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.635#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200814_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:40.86 +18:00:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.693 3350284291443501952 090.67069155634 +18.00676592692 13.0096 12.5148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200815_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200815_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:30.61 +11:14:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.325 3342087019941734784 089.37719661488 +11.24462500106 13.0419 12.6948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.325#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200816_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:53.63 +15:42:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 4.593 3348095099371591168 087.47315297195 +15.70692516451 12.6438 12.1920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200819_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200819_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:49.89 +11:40:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.994 3342957459492164480 089.20774551914 +11.67856443397 12.7312 12.2653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200821_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200821_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:19.18 +14:12:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.796 3345175827279012224 091.33039300686 +14.21027805006 13.1116 12.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200822_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200822_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:23.40 +17:37:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 5.777 3373477973834339328 092.09763390040 +17.63173370806 12.1002 11.0310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200823_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200823_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:48.43 +10:13:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200824_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200824_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:33.07 +15:12:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.418 3345006433769473152 093.88755384839 +15.20812765193 13.0634 12.4369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.418#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200828_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:53.10 +13:04:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 4.598 3344101089024476160 093.97108709394 +13.06992724579 12.7597 12.2443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.598#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200829_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:32.31 +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 200830_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200830_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:18.42 +15:07:36.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)
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Considering the candidate 200831_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200831_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:11.23 +14:32:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.715 3348426907065674496 090.04698014769 +14.53414740740 12.8398 12.3311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200835_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200835_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:41.16 +15:50:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.368 3348111488966539008 087.92144800561 +15.83784317950 12.2328 11.4364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200836_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200836_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:11.26 +16:10:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 5.861 3345887623619012736 093.54680330667 +16.16512556569 12.5646 11.7946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.861#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200837_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:26.34 +11:35:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.622 3331837033249603712 093.36004479014 +11.59155469199 12.2866 11.2188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.622#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200838_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:05.29 +14:02:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.827 3347025274558597504 087.77212076487 +14.04549476456 12.6176 12.1463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.827#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200839_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:27.45 +17:54:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200840_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200840_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:47.04 +12:13:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.580 3343201757231045248 087.69588515421 +12.21553816911 12.5120 11.9390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200842_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200842_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:12.71 +15:24:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 4.089 3348722435181321984 089.30298874626 +15.40647573700 13.0135 12.5762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200846_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200846_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:51.42 +15:52:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 5.669 3368935204108493184 095.96416624453 +15.87867727057 12.6190 12.0750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.669#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200849_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:21.18 +10:11:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.862 3327655040771108736 098.58813851330 +10.19118888818 13.1780 12.7292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200850_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200850_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:53.81 +17:55:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 3.845 3350244434147448960 089.72428424972 +17.91996228641 12.7755 12.2702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.845#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200851_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:02.57 +15:00:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.615 3347202158489229696 089.01028924039 +15.00045035307 12.4937 11.7723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.615#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200853_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:36.84 +17:53:12.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)
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Considering the candidate 200855_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200855_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:17.62 +16:09:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 5.683 3368967334760146560 096.32332009104 +16.16086869320 12.2561 11.3997 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 200856_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200856_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:19.65 +14:13:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.012 3356440113449222528 097.08143008752 +14.21572250391 11.8154 10.6198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.012#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200857_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:41.86 +09:56:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.606 3330448212625683072 095.92405124128 +09.94226088192 12.3144 11.3842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.606#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200858_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:56.53 +14:42:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.901 3346991838232847744 089.23554296276 +14.71527762171 12.2346 11.4939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200859_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200859_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:22.23 +11:33:14.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
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Considering the candidate 200860_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200860_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:29.64 +14:45:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 5.346 3344837413921531520 093.87339326052 +14.76299093228 12.2147 11.3601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.346#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200861_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:14.18 +13:23:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 5.147 3343611836409867776 090.55934277124 +13.39203724678 12.5807 12.3331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.147#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200864_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:42.95 +13:25:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.315 3343750069937229696 089.42874704002 +13.42896355669 12.4048 11.7110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.315#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200865_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:59.34 +17:48:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 4.293 3369781724979663744 096.74716619232 +17.80617132422 12.3751 12.0085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200866_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200866_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:42.70 +12:40:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 3.769 3343278173290186752 088.67786817265 +12.67637075116 12.2889 11.7990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200873_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200873_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:40.44 +17:17:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 4.320 3369748125454987392 096.66853947125 +17.29674516671 12.1125 11.3303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200874_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200874_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:44.92 +16:35:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 3.016 3358683495127303040 099.68713909596 +16.58366262296 12.2463 11.4557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200875_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200875_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:09:11.75 +15:26:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 5.680 3345908647480814080 092.29934639249 +15.43716177382 12.6420 12.0956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200880_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200880_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:33.70 +15:30:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 4.216 3345604495077648384 091.39063937143 +15.50632099519 12.2968 11.7786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.216#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200881_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:43.96 +09:59:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.323 3330486764252050560 095.18324824757 +09.99275239639 12.1649 11.9792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200883_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200883_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:48.81 +16:28:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.951 3349697878087629184 089.20341727050 +16.47918098784 12.1159 11.6774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200884_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200884_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:10.86 +13:33:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 4.103 3346441880559578368 087.79522024758 +13.56041623763 11.8536 11.2904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200885_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200885_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:40.46 +11:48:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.363 3337148529106292224 087.41806972761 +11.80910156059 12.0512 11.2523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200888_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200888_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:15.64 +16:47:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 3.849 3349766387108428544 089.06506399157 +16.79401874301 11.7978 10.9640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200889_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200889_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:40.59 +16:33:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 4.722 3346157794242075520 092.66905550907 +16.56060671619 11.6076 10.7309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200892_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200892_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:02.80 +10:58:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 3.243 3330233837918786432 091.76165733696 +10.97582150484 11.7920 10.9674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200893_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200893_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:30:28.15 +16:59:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 4.631 3369479565442237312 097.61689195553 +16.99785494787 12.1899 11.9093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.631#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200898_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:18.81 +11:30:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 2.823 3328081921862272384 098.82825432242 +11.50141915759 11.6717 11.2658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.823#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200900_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:24.46 +13:52:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 3.732 3344576554784151936 093.85155570202 +13.86607978512 12.1268 11.6565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.732#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200901_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:22.45 +11:46:45.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)
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Considering the candidate 200902_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200902_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:47.31 +13:09:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 2.546 3355399391336685696 098.69663990043 +13.16233481249 11.7429 11.2973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200903_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200903_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:05.27 +17:19:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200906_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200906_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:22.72 +14:04:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 3.120 3343905955772961152 089.84487003571 +14.08010042817 11.4251 10.6755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200907_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200907_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:48.45 +09:57:26.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)
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Considering the candidate 200911_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200911_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:06:54.10 +14:27:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 3.768 3345280109085235712 091.72596360951 +14.45945834120 11.4078 10.9626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200912_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200912_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:41.80 +16:32:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 3.164 3369541211110732672 096.42382454315 +16.54082334187 10.9869 10.2679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200913_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200913_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:50.66 +13:59:02.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)
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Considering the candidate 200914_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200914_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:25.72 +16:03:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 2.994 3357845053090488832 100.35714121559 +16.06408544540 11.0387 10.6139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.994#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200915_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:26.95 +17:16:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 2.503 3349986323792979328 088.86212951416 +17.27215543188 11.0935 10.8277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.503#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200916_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:17.81 +15:55:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 3.134 3345875838228836480 093.32432743061 +15.91797045444 11.0973 10.7666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 200920_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200920_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:18.63 +14:00:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.06, MAG_FAINT_SEARCH_LIMIT=10.04)GAIADR2_OUTPUT=# 0.994 3345194347178716800 092.07770715289 +14.00376444567 8.3071 7.1898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.994#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 200921_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:32.07 +13:58:00.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 200922_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 200922_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 201018_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201018_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:15.48 +15:33:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 2.286 3345750115942949120 092.81452392098 +15.56272641147 10.3958 9.9883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.286#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201023_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:18.70 +13:59:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 2.704 3345194347176271872 092.07802470555 +13.98856167066 10.5449 10.4762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201053_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201053_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:35.84 +11:51:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.36, MAG_FAINT_SEARCH_LIMIT=11.34)GAIADR2_OUTPUT=# 2.422 3352113986172044928 099.14889968554 +11.85436674720 10.7155 10.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201067_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201067_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:25.29 +15:43:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.48, MAG_FAINT_SEARCH_LIMIT=11.46)GAIADR2_OUTPUT=# 1.176 3357096216952323968 098.85533171442 +15.71842612673 10.4561 9.7252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201118_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201118_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:05.16 +15:12:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 2.633 3348478657131124480 090.52162924754 +15.19941809654 10.6687 9.8662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201186_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201186_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:31.86 +15:24:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.17, MAG_FAINT_SEARCH_LIMIT=12.15)GAIADR2_OUTPUT=# 4.139 3345596970294948224 091.38319239071 +15.41096001526 11.3839 11.2618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201191_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201191_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:00.00 +18:04:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 2.752 3350286009430416896 090.75017501953 +18.06644822458 11.2410 11.0507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201205_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201205_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:35.21 +11:13:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.745 3342086745063828096 089.39667657019 +11.22137743822 11.2684 10.7571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201241_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201241_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:44.09 +16:56:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 2.679 3349354791800163072 090.43370513177 +16.93625582270 11.1866 10.4013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201259_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201259_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:52.47 +17:20:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.463 3370453148628289792 095.21855338735 +17.34845814795 11.3304 10.8012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201290_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201290_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:25.59 +13:44:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201295_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201295_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:43.93 +16:47:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 2.082 3369392296004628736 096.93299990475 +16.78342297646 10.8171 9.7201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201334_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201334_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:53.90 +17:16:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 4.023 3349388949677927296 090.97458706794 +17.27949370533 11.7662 11.4565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201343_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201343_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:25.19 +13:26:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 1.102 3343604281566297728 090.35498295526 +13.44963933601 11.8865 11.1545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201354_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201354_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:44.99 +11:17:01.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 201360_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201360_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:06:33.28 +16:49:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 4.601 3349206327668085504 091.63881200775 +16.81747961446 11.6869 11.0212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201368_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201368_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:19.09 +17:40:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 3.248 3350026528984261632 089.07931686384 +17.66681788967 11.5881 10.9490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201431_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201431_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:26.76 +15:43:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 3.249 3348086264620416256 087.86177490020 +15.72166490026 12.0083 11.6320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201461_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201461_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:01.72 +10:51:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 4.768 3336839501915593600 087.25715516966 +10.85736991660 11.8198 11.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201487_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201487_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:09:59.34 +16:45:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.504 3349167015830923776 092.49717291038 +16.75683508035 11.8807 11.3393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201492_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201492_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:54.78 +17:41:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 4.396 3369776987634402176 096.72833246704 +17.69719812288 11.9736 11.4653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201505_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201505_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:48.75 +10:25:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 5.027 3336752464402088576 087.95297007775 +10.42713959719 12.0271 11.3473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201533_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201533_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:53.30 +17:47:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.264 3369792483876730880 097.22206187216 +17.79278797109 11.8663 11.0490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201566_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201566_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:26.40 +13:30:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.824 3332545080078277120 095.35960441075 +13.51095521187 11.9295 11.0255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201583_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201583_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:52.95 +16:26:13.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 201605_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201605_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:45.56 +13:50:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.497 3346642747589641472 087.68980554282 +13.83755671432 12.1733 11.6438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201671_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201671_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:34.55 +14:02:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201673_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201673_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:06:34.12 +16:48:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 5.585 3349206117214115328 091.64227933264 +16.81098027263 11.6160 10.4880 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201690_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201690_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:50.44 +16:42:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 5.371 3349145300476276608 092.20999595535 +16.70776690786 12.2595 11.5481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201697_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201697_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:50.92 +17:12:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.484 3358825503925493760 100.46173302454 +17.20315310497 12.3347 11.9111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201700_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201700_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:04.44 +18:10:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.223 3371164051614650752 098.76870459185 +18.17298708281 12.1652 11.3874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201703_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201703_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:27.01 +17:10:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 4.826 3370388449239528448 095.61265851950 +17.17588643624 12.1563 11.7205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201706_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201706_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:19:35.92 +16:11:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 4.230 3369111125966694272 094.89945935501 +16.18923088560 12.2352 11.7144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201710_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201710_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:17.25 +16:32:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 4.470 3348917083093093632 090.32177078968 +16.53909581331 12.4054 12.0390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201723_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201723_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:17.03 +15:47:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.982 3348803111840941696 088.82124704033 +15.79662379989 12.3597 11.5905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201730_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201730_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:10.72 +14:28:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 4.276 3344825735905847168 093.54439435012 +14.47300843745 12.3357 11.8265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201736_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201736_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:17.34 +10:01:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201740_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201740_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:33:20.22 +18:02:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.645 3371081897479858048 098.33438876504 +18.04146638911 11.8644 10.8017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201752_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201752_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:32.40 +13:10:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 4.554 3346360546762559104 088.38504790172 +13.16795797092 12.3235 11.7916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201766_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201766_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 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=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201772_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201772_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:36.63 +12:31:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.020 3346213796319467648 087.65251774708 +12.53111204603 12.5088 12.1550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201785_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201785_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:17.64 +11:05:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.851 3342069397692976768 089.57359010533 +11.09829426935 12.5386 11.9642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201823_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201823_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:58.70 +15:28:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.339 3345591747613893376 091.49468762610 +15.47852124743 12.1418 11.2297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201869_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201869_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:20.04 +11:40:04.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201871_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201871_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:47.19 +10:18:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.846 3341813619502378240 090.69619107494 +10.31602142529 12.8673 12.3681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201880_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201880_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:58.33 +17:17:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 4.614 3369657965500857984 096.49314948059 +17.28369462775 12.1505 11.1256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201895_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201895_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:57.33 +15:39:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 5.183 3357232693834767360 097.48871068355 +15.65001346320 12.4718 12.0006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201906_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201906_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:32.81 +17:28:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.852 3359023042361110272 100.13650757046 +17.46780481902 12.7382 12.1493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201935_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201935_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:24.07 +14:06:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 4.155 3343906063148807040 089.85029497556 +14.10465139972 12.5161 11.9505 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201943_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201943_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:36.46 +13:46:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.838 3344520037313447936 094.15143681526 +13.77546184342 12.8852 12.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201944_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201944_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:50.67 +15:25:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 4.764 3347286649087380736 088.46104249624 +15.42429021899 12.7016 12.3284 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#
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Considering the candidate 201949_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201949_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:30.52 +16:25:09.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 201988_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201988_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:45.88 +12:05:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201994_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201994_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:31:02.40 +16:57:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 4.489 3369454796368516480 097.75982259933 +16.95657018374 12.5728 12.0889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201996_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 201996_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:24.13 +12:58:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.339 3343522264871210240 090.60082052875 +12.97688126822 12.6861 12.2533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202026_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202026_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:32.07 +16:35:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.949 3349712236160778112 089.13357613302 +16.58379294168 12.6162 12.0249 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 202037_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202037_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:24:33.27 +13:00:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 5.267 3332266186381166080 096.13837478976 +13.00305737560 12.8746 12.4125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202043_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202043_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:30.51 +11:22:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.744 3342842556227533696 089.12709839198 +11.37126581374 12.6524 12.1520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202044_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202044_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:38.00 +14:27:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 5.348 3355976123841683072 100.15861974061 +14.45148491578 12.7423 12.4904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202060_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202060_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:08.46 +15:03:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.087 3348484601365627776 090.03541349476 +15.06454031990 12.7473 12.3633 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202062_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202062_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:28.01 +12:53:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 5.633 3346325057449619840 088.11692928040 +12.88428363636 12.8257 12.4507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202067_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202067_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:09.29 +13:52:43.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202070_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202070_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:20.96 +13:38:22.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202074_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202074_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:39.07 +18:04:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 4.972 3371264897445816704 098.16268778843 +18.07215031061 12.6055 12.2284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202077_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202077_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:33.77 +16:11:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 5.399 3346112954783949312 092.64047008736 +16.18848996232 12.5471 11.6939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202094_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202094_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:05.57 +16:43:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.762 3349720589874563968 089.27344231483 +16.71714082128 12.7106 12.1629 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202097_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202097_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:06.33 +16:33:35.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)
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Considering the candidate 202106_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202106_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:15.05 +17:30:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.595 3369720912541847296 097.31247712788 +17.50477058305 12.6315 12.0607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202116_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202116_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:33.22 +17:33:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 5.131 3373251684895191168 093.13838267387 +17.56485293110 12.7419 12.2267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202126_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202126_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:48.50 +13:31:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.927 3344168640269409920 093.20203572497 +13.51754871453 13.0075 12.6339 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202128_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202128_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:37.58 +15:34:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 5.705 3348606131759642112 091.15654701349 +15.57666566456 12.6935 12.2511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202131_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202131_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:43.33 +18:12:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.173 3370569563719615104 096.93057530962 +18.20300784835 12.5903 11.9228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202137_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202137_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:17.74 +14:55:18.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 202138_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202138_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:04.68 +12:36:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.537 3342748827159782272 090.76955879872 +12.61126892587 12.8299 12.3382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202145_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202145_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:22.86 +13:08:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.432 3346368213280601088 088.09539984189 +13.13538718664 12.7517 12.0042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202156_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202156_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:19.73 +13:11:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 5.329 3346404767743098880 087.33200740963 +13.18469935554 12.5569 11.7444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202157_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202157_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:11.25 +13:28:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 5.103 3344188117941795328 093.29695687676 +13.48089033685 12.4364 11.5593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202158_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202158_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:56.69 +12:59:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 4.427 3342776795986519680 091.48619042234 +12.98424270358 12.6805 12.2078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202161_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202161_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202166_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202166_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:06.54 +12:58:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.563 3344089887749562624 093.52687633102 +12.96714694997 12.6271 11.8167 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#
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Considering the candidate 202171_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202171_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:52.77 +17:32:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.733 3370438756195767168 095.71992116925 +17.54374160170 12.9709 12.5361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202182_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202182_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:25.47 +16:58:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.136 3349740724680896128 089.85596284808 +16.97452630478 12.5659 11.7051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202183_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202183_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:41.97 +10:55:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.168 3342013391319536640 089.42479045164 +10.91659520686 12.8175 12.2907 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 202193_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202193_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:47.29 +11:53:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.117 3331858400708743296 093.94661868605 +11.89198948583 12.9382 12.3509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202209_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202209_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:00.74 +12:28:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.954 3343257557447133184 089.00299742522 +12.46643385548 13.0756 12.8794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202257_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202257_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:51.14 +13:51:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.027 3346795510987201920 088.71351314086 +13.85452006185 12.9355 12.5218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.027#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202258_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:13.67 +15:20:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.832 3345012717303573376 093.80695057044 +15.34038013426 13.0408 12.5691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202272_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202272_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:48:14.41 +15:36:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.336 3348189382493112320 087.05942919569 +15.60786860225 12.6739 12.0459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202274_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202274_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:20.27 +13:08:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 4.980 3346368277701929728 088.08453618645 +13.14847999423 12.8927 12.4001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202275_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202275_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:19.40 +13:11:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 4.754 3344249763610589184 092.58101034558 +13.19807976003 13.0992 12.5818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202292_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202292_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:37.40 +18:05:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.509 3370598730838491264 095.90613188866 +18.09369680463 12.9520 12.4070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202293_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202293_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:27.58 +14:46:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.781 3344837486936182912 093.86443664937 +14.77100567174 12.9905 12.5320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202331_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202331_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:53.33 +16:19:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.605 3358606052576070784 100.47161039489 +16.32252345597 13.4634 13.0275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.605#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202335_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:23.14 +15:49:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.835 3348064519204708992 088.09616932128 +15.81598930374 12.8109 12.2654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202336_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202336_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202338_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202338_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:22.78 +14:22:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202340_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202340_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:06.32 +17:09:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.510 3349760928207104000 089.52620984621 +17.15442108860 12.6940 11.7654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202360_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202360_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202361_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202361_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:04.30 +17:22:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 5.262 3359019297149615744 100.26791964743 +17.37403841393 12.8089 12.0202 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 202370_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202370_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:48.88 +18:17:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.586 3373528967983878912 092.70327976722 +18.29677016067 12.8483 12.3800 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#
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Considering the candidate 202372_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202372_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:45.60 +16:34:18.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 202374_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202374_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:28.17 +16:25:11.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 202386_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202386_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:03.61 +15:41:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 4.733 3348763976098955776 089.51521611652 +15.69736277212 13.0586 12.5587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202389_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202389_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:54.38 +11:58:21.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 202392_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202392_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:06:22.04 +10:45:15.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 202393_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202393_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:18:39.55 +17:35:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.492 3370290665722797824 094.66447383406 +17.59444925488 13.0097 12.5044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202395_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202395_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202398_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202398_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:09.40 +13:38:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.112 3346765274417578880 088.53885976439 +13.63239738016 12.9168 12.1783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.112#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202407_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:14.75 +16:34:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.195 3349058198540181760 091.81163502854 +16.56617794186 12.8725 12.2819 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#
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Considering the candidate 202414_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202414_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:23.38 +13:50:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.738 3344429052725516928 092.59752528287 +13.83418932603 11.2198 9.8179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202415_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202415_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:12.23 +11:14:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.551 3342870529353525632 088.30102247681 +11.24718181503 13.0267 12.3759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202423_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202423_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:54.63 +11:04:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.591 3342057577942876672 088.97765909997 +11.08128069186 12.9648 12.4305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.591#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202425_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:49.85 +13:38:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 5.403 3343853144854246784 089.70735625011 +13.64428855046 13.1372 12.5806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202426_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202426_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:38.65 +15:45:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 5.763 3369068799066487936 094.41054549919 +15.76138858278 13.1102 12.6108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.763#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202430_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:15.82 +09:57:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.286 3336640176776475136 087.56561476189 +09.95686772871 13.0296 12.4604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202470_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202470_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:46.87 +17:35:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.609 3350208326359314176 089.44609958617 +17.59735799575 13.1928 12.6883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202478_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202478_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:24:40.75 +17:23:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.348 3369668548300338176 096.16947898442 +17.38791309686 12.8737 11.9815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202481_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202481_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202483_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202483_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:06:34.20 +15:33:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.875 3345969056199793024 091.64250816233 +15.55045144262 12.5929 11.6569 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 202503_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202503_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:42.59 +12:17:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.560 3343195091441390464 088.17746570654 +12.29476105520 12.8012 11.9325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.560#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202505_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:26.09 +16:10:13.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 202508_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202508_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:34.60 +11:46:42.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)
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Considering the candidate 202510_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202510_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:59.87 +14:14:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202536_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202536_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202538_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202538_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202549_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202549_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202553_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202553_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:43.04 +18:02:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.868 3370702943926205312 095.17934314625 +18.04181447075 12.5599 11.6093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202567_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202567_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202571_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202571_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:30.45 +11:00:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.365 3330254762997242112 091.87675871697 +11.01165296275 12.6619 11.8391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202575_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202575_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:57.74 +17:51:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.685 3350418981618210304 088.99048454188 +17.85720204125 12.9885 12.4559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202578_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202578_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:06:20.00 +14:26:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.483 3345279181372314624 091.58377857882 +14.44006689857 13.1161 12.6793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202584_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202584_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:03.32 +13:39:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.442 3332364317793274368 096.51348785808 +13.66183163531 12.3351 11.2653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202593_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202593_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202596_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202596_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:49.50 +17:20:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.422 3349815147874197248 089.45580863539 +17.34113746329 13.1921 12.6949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202608_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202608_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202609_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202609_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:34.28 +13:26:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202611_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202611_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:43.29 +15:24:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202612_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202612_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:02.65 +15:13:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.619 3347971610471158016 087.26088491716 +15.22466875216 13.3239 12.9848 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 202616_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202616_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202619_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202619_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:12.14 +15:48:00.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 202625_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202625_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:29.59 +15:06:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202630_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202630_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:40.06 +11:53:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.792 3342932681823339520 088.66668105157 +11.89135554383 13.1100 12.2864 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#
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Considering the candidate 202641_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202641_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:41.27 +13:46:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.594 3346650100573394944 087.42187520447 +13.77192078285 13.1659 12.6057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202644_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202644_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:52.10 +18:15:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.753 3350312947466883712 090.96696986183 +18.25223973825 12.7086 11.6825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202655_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202655_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:09:21.71 +13:07:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 5.132 3344245777880783360 092.34027427484 +13.12439119931 13.2273 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202656_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202656_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:53.52 +17:20:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.359 3370266197291202560 093.97277893926 +17.33905411562 12.7462 11.8069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202670_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202670_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:52.97 +13:12:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.615 3332287863076193536 096.97045689800 +13.21215841381 12.9135 11.8493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202671_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202671_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:57.34 +15:37:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 5.386 3345805740064507776 093.73884263204 +15.63167212358 13.1680 12.7977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202674_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202674_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202677_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202677_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202684_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202684_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:43.88 +16:41:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202690_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202690_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:24.84 +17:53:06.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202705_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202705_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202729_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202729_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:15.95 +13:13:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.020 3344111018988845440 094.06606377346 +13.23196502846 13.3168 12.7369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202749_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202749_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:52.86 +14:21:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 5.114 3345268697353714688 091.97024192916 +14.36113502853 13.1894 12.6523 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 202751_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202751_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:24.18 +18:05:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.847 3370566398327364352 096.85066233207 +18.09629582934 13.1704 12.7036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202758_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202758_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:23.30 +15:56:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.704 3348119322987332480 088.09684072008 +15.94863088749 12.9684 12.1466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202761_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202761_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:05.00 +10:00:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202763_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202763_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:14.37 +15:48:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202764_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202764_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:52.85 +14:11:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.302 3346857289796673536 088.72123456578 +14.19383800812 13.1792 12.6928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202770_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202770_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:43.61 +12:19:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.627 3342641384257644416 090.68148577155 +12.32261880052 13.3530 12.9573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202775_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202775_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:39.96 +16:32:42.3 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 202781_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202781_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:30:07.13 +15:49:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.790 3357239733282561920 097.52922975603 +15.82291826523 13.3394 13.0460 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 202783_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202783_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:08.35 +10:34:29.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202790_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202790_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:53.05 +17:36:46.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 202793_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202793_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:19.39 +15:25:19.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
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Considering the candidate 202797_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202797_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:09.78 +13:32:26.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 202798_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202798_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:19.40 +17:13:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 5.137 3369691221428831872 097.08045195488 +17.23070353826 13.2581 12.9854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202802_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202802_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:17.09 +15:54:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.830 3345875735149626496 093.32103278618 +15.90202815244 13.3038 12.9097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202806_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202806_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202810_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202810_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:17.86 +12:37:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 5.121 3343268071527371904 089.07469468226 +12.62635347700 13.3578 13.1338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.121#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202822_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:44.10 +12:49:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.807 3344069611204146176 093.43356318317 +12.81631612254 13.6079 12.7357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202836_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202836_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:39.69 +16:37:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.833 3348953783592272128 089.66634880272 +16.61765141382 13.5213 13.1340 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 202838_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202838_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:27.85 +17:09:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.832 3370223286275686912 093.36551705681 +17.16326493666 13.3028 12.7817 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202839_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202839_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:33.74 +16:11:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202842_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202842_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:08.39 +14:27:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 5.629 3344825697247558912 093.53455522839 +14.46312490704 13.1439 12.6068 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 202856_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202856_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:29.63 +15:49:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.288 3357250767057119104 097.37309398805 +15.82693469515 13.2807 12.8444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202857_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202857_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:14.13 +12:48:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.845 3332062226974934016 093.80848461812 +12.80225490251 13.4990 13.0291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202860_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202860_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:33:49.40 +18:00:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.222 3371078053487168128 098.45570931479 +18.00055422262 13.2296 12.7323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202861_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202861_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:00.98 +16:09:33.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202863_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202863_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202865_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202865_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:25.94 +16:37:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.354 3348967527487529984 090.10796848440 +16.61973906657 13.4662 12.9271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202869_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202869_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:00.32 +14:23:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.441 3347073103313554816 088.00052194638 +14.39713257143 13.5401 13.1927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202871_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202871_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:02.84 +10:18:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.358 3341770021292829056 089.76170346899 +10.30246149553 12.9572 12.0882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202877_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202877_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:38.04 +11:43:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.158 3337144650752350592 087.40814769082 +11.72477610187 13.1398 12.3465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202878_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202878_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:49.23 +11:06:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.429 3330118664073573632 093.20449162710 +11.11241052929 13.3048 12.9786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202895_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202895_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:58.10 +11:31:05.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 202896_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202896_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202899_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202899_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:09.66 +12:56:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.409 3346329214977679232 088.04014277091 +12.93847411677 13.1262 12.3577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202900_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202900_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:39:11.74 +16:28:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.084 3358670030408653952 099.79873430757 +16.47823742762 13.1420 12.4792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202910_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202910_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 202927_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202927_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:24.61 +13:27:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202933_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202933_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:06.02 +12:01:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 5.330 3342456494506035456 092.02486039460 +12.01550775189 13.3408 12.7272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202937_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202937_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:21.86 +17:27:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202949_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202949_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:36.47 +10:30:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202951_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202951_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:47.61 +13:22:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.687 3343596962942083328 090.19836078039 +13.37261480968 13.2596 12.4468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202956_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202956_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:13.52 +15:43:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.485 3348792292822869248 089.05633156261 +15.73200422078 13.3905 12.8816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202962_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202962_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:13.64 +13:05:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.695 3355354143858801920 099.05650124562 +13.09631246794 13.3134 12.8561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202964_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202964_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:16.37 +17:30:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 5.243 3369720946901581056 097.31823966737 +17.51023825738 13.1093 12.7794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202968_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 202968_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202969_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202969_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:41.52 +15:32:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202973_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202973_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:12.75 +14:42:00.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)
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Considering the candidate 202985_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202985_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:48.60 +12:49:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.146 3344072467362456960 093.70196302565 +12.82783661078 13.4893 13.1232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202989_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202989_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:57.64 +11:08:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.726 3330119179469646848 093.23963625886 +11.13874425129 13.0992 12.2623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202994_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202994_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:30.92 +12:02:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.600 3331910460010031872 093.12884269174 +12.03708330347 13.5084 12.9388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202998_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 202998_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:00.79 +12:52:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.484 3343473572823139328 090.00396463441 +12.87934750069 13.4151 13.0810 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 203007_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203007_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:09:17.15 +14:34:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.178 3345249765138904064 092.32132783419 +14.56862277810 13.4202 12.8205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203020_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203020_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:05.93 +16:07:26.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 203025_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203025_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203030_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203030_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:11.67 +17:24:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 5.883 3349266968308888704 092.04790576534 +17.40426687181 12.6820 11.5695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203033_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203033_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:04.05 +09:55:16.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 203035_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203035_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:09:28.51 +17:28:06.4 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 203039_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203039_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203046_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203046_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:43.45 +10:00:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203050_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203050_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:38.93 +12:49:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.780 3344069787302738176 093.41167930308 +12.81603509804 13.5519 12.6857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203055_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203055_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:33.50 +18:11:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.372 3350310782801774336 090.88997905288 +18.18745646460 12.5078 11.2665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203065_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203065_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:37.98 +13:10:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203072_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203072_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:52.60 +10:38:04.0 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 203073_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203073_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:38:13.55 +17:47:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203077_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203077_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203081_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203081_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:23.41 +13:54:27.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 203087_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203087_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203093_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203093_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203096_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203096_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203099_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203099_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 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=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)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 203111_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203111_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:00.70 +14:58:53.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)
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Considering the candidate 203113_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203113_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:16.27 +15:59:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.899 3369278015515633536 096.81775023110 +15.99550090228 13.5854 13.1927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203115_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203115_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:38.08 +14:13:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.381 3344475507091417088 092.65872944011 +14.22806206946 13.4306 12.8439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203117_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203117_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203122_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203122_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:03.57 +13:39:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.714 3332364141695350912 096.51479192999 +13.65224819165 13.0188 12.1662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.714#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203123_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203131_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203131_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:59.15 +13:01:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 5.112 3343712583462968448 088.99626854998 +13.02953666856 13.2761 12.7180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203132_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203132_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203138_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203138_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203140_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203140_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203144_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203144_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203150_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203150_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:56.55 +18:09:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.638 3370707861667708544 095.48502870894 +18.15088560933 13.2770 12.2382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203155_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203155_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203157_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203157_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203162_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203162_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:21.34 +17:00:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.462 3349743782697604864 089.83823275346 +17.00404764242 13.4454 12.9351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203173_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203173_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:23.23 +14:59:09.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 203175_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203175_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:01.29 +12:54:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.829 3332079887880225920 094.25486750302 +12.91422536403 13.6903 13.1067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203180_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203180_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:09:00.36 +14:09:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.554 3345203143271695872 092.25140588413 +14.15845999959 13.5138 13.0777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203184_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203184_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:00.83 +13:55:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.174 3355696259473513472 098.00353090324 +13.92792591042 13.4473 12.9059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203190_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203190_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203191_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203191_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203203_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203203_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:02.54 +11:51:52.6 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 203204_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203204_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:46.71 +16:49:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.457 3369393567314931712 096.94451270717 +16.82693324043 13.3832 12.8503 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 203205_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203205_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:59.89 +17:51:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 5.363 3369805609296408192 096.74965402426 +17.86176422134 13.2262 12.4675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203208_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203208_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203211_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203211_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:41.84 +11:46:48.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
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Considering the candidate 203225_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203225_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:07.65 +17:23:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.149 3371019263975178112 098.03178249040 +17.38576768475 13.3216 12.5217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203227_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203227_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:10.40 +16:00:20.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 203239_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203239_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:17.05 +12:54:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203240_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203240_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:32.80 +11:02:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.880 3342057165623036800 088.88687714913 +11.03240769550 13.3639 12.4754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203241_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203241_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:46.09 +17:15:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 3.717 3349798444741963648 088.94184217360 +17.25265199484 13.3446 12.4932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203250_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203250_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:39.25 +14:41:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 5.340 3347164019181859200 088.66305712862 +14.69117599099 13.0585 12.0422 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 203257_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203257_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:46.08 +17:35:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203263_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203263_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:49.70 +13:49:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 5.429 3346830106945060480 087.95701030772 +13.82257681677 13.3339 12.7810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203267_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203267_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:30:25.22 +17:20:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.462 3369526603925834240 097.60511374302 +17.33440007229 13.4532 12.6703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203268_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203268_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203271_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203271_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:56.60 +16:10:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 4.823 3357146343513112448 099.23588849036 +16.17757802501 13.4066 12.5658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203272_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203272_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:17.53 +12:14:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203276_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203276_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:42.91 +14:21:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 4.887 3347060321491428736 088.17848411495 +14.34987015175 13.3409 12.5665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203281_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203281_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:43.89 +16:12:34.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
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Considering the candidate 203290_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203290_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203292_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203292_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:25.17 +14:31:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203294_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203294_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:57.40 +13:03:21.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 203295_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203295_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:43.95 +14:52:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.242 3344903491993372928 093.43316697895 +14.86976664965 13.6193 13.2605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203299_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203299_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203305_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203305_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203323_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203323_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:04.93 +17:44:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.978 3359043177167723392 100.02020497712 +17.73452956759 13.9351 13.4566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203329_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203329_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203340_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203340_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 203345_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203345_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203350_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203350_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203356_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203356_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:52.78 +16:28:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 5.483 3369216507285239296 095.21999695578 +16.47278443316 13.4907 12.9752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203361_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203361_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:38.42 +15:49:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.403 3348070287343236352 088.16025482766 +15.82486935417 13.4816 13.0020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203363_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203363_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:31.61 +10:48:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.756 3341999883644048128 089.88111600940 +10.81266161092 13.1970 12.2588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203366_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203366_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:48:39.61 +10:58:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.487 3337033462639557760 087.16493205109 +10.98200966142 13.5477 12.9816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203372_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203372_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203373_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203373_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:52.23 +10:13:56.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 203375_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203375_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:19.09 +17:08:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 5.276 3349805247975323392 089.32883161573 +17.14045093874 12.8013 11.6138 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 203377_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203377_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:44.93 +13:06:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 5.743 3332283297530696832 096.68762104408 +13.10270616573 13.2714 12.4362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203391_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203391_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:29.05 +13:52:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.320 3343831846114180736 090.37014081620 +13.86848821976 13.9660 13.1220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203400_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203400_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:57.54 +09:49:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203403_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203403_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203407_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203407_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:25.81 +16:23:16.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 203408_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203408_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:23.63 +10:44:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.505 3341890280378126464 090.34846684556 +10.73772091921 13.7368 13.4181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203414_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203414_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:29.16 +13:54:39.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 203415_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203415_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203420_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203420_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203423_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203423_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:25.43 +11:56:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.337 3343155955700023168 087.60605152246 +11.93904880634 13.6624 13.1135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.337#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203431_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:05.44 +17:21:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.098 3370453389145548160 095.27237363168 +17.35522975346 13.6181 13.1831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203434_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203434_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203436_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203436_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:45.54 +16:35:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 5.240 3348952924598815488 089.68976818892 +16.58873912473 12.9994 12.0436 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 203445_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203445_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:34.80 +14:12:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.267 3346855842388596352 088.89559670250 +14.20341201561 13.4739 12.8761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203446_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203446_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203458_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203458_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:50.41 +17:51:29.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 203460_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203460_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203463_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203463_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203470_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203470_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:56.95 +17:52:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.771 3350407544123197056 089.48629840031 +17.87882133075 13.4224 12.4898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203475_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203475_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:17.45 +11:37:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203481_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203481_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:12.07 +11:17:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.030 3337068406493385728 087.54956317409 +11.28563255882 13.5655 12.9609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203487_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203487_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:40:04.18 +16:12:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203490_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203490_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:24.50 +16:18:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.702 3357371850774022400 098.10201780105 +16.31130638763 13.0454 12.0051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.702#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203492_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203515_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203515_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:44.11 +13:56:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203518_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203518_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203519_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203519_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:52.42 +13:36:29.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 203528_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203528_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203530_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203530_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:34.06 +11:02:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.077 3341915981461934592 090.39181586672 +11.04542746453 13.5229 12.6909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203536_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203536_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:42.29 +17:12:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203537_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203537_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:20.16 +12:15:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.396 3343378263207910656 089.83334310327 +12.25587798965 13.4157 12.6307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203539_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203539_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:38.74 +13:05:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 5.076 3344060540234743552 092.66067047068 +13.09820837622 13.7982 13.2259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203557_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203557_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:32.56 +13:10:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.721 3346395872869652736 087.63533661239 +13.17355481623 13.5551 13.0582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203558_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203558_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203559_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203559_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:33.41 +16:48:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.642 3369250321564569600 095.63932947051 +16.79996484798 13.4978 12.8227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203565_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203565_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:48.25 +15:23:34.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 203566_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203566_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203569_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203569_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 203572_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203572_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:36.98 +14:40:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 5.373 3347872345187595520 087.40284980173 +14.66771469263 13.6313 13.0201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203573_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203573_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:17.20 +12:35:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 5.631 3346220844361968640 087.82172887290 +12.58604808586 13.5963 13.2071 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#
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Considering the candidate 203588_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203588_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:53:10.80 +15:22:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.770 3347287576800029184 088.29559277758 +15.36803918572 13.7881 13.2797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203590_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203590_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:16.46 +15:16:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.875 3347227206739949568 088.81828406502 +15.26909363616 13.6108 13.1519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203593_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203593_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:30.32 +11:35:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.440 3337140974260785408 087.37602155482 +11.58538122826 13.6127 13.0112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203594_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203594_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:24.82 +15:45:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.361 3348799920684849408 088.85319716402 +15.74958133421 13.4864 13.0783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203597_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203597_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:38.85 +15:42:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 5.467 3369030208782864768 095.16164666202 +15.69908082032 13.4126 12.7424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203602_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203602_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203603_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203603_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:45.36 +13:40:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203613_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203613_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:33.69 +17:04:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.982 3349794291512878592 088.89081554739 +17.06736612998 13.7714 13.4247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203622_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203622_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203626_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203626_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:44.51 +09:59:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.787 3341742327344196224 089.68440222902 +09.98843604958 14.3627 13.4643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203629_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203629_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:56.47 +16:11:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.952 3357146347810392064 099.23479689737 +16.18373693002 13.4610 12.9240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203636_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203636_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:07.34 +12:35:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.924 3343267723631107456 089.03078684812 +12.59695608819 13.6855 13.2261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203649_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203649_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203650_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203650_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:27:05.01 +17:21:30.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 203664_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203664_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:47.09 +17:02:49.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 203675_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203675_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 203676_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203676_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:30.83 +16:22:25.7 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 203677_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203677_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203679_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203679_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203681_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203681_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:43.01 +17:35:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.444 3350164826930635264 090.42881118218 +17.58981371026 13.3657 12.7481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.444#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203689_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:35:10.14 +12:37:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 5.440 3355225672796911104 098.79222552796 +12.62498914517 13.2827 12.7618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203690_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203690_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:51:59.50 +15:38:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203700_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203700_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:00.51 +14:22:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.405 3346917488059002624 089.75326536911 +14.36716804620 13.7002 13.1066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203707_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203707_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203717_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203717_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203721_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203721_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203724_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203724_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:36:45.19 +14:33:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 5.598 3356132460651403008 099.18838350362 +14.55508651825 13.4724 13.1675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203731_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203731_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:32:09.25 +17:17:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.678 3369513792039011328 098.03791458587 +17.28594988516 13.7527 13.1458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.678#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203733_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203737_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203737_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203740_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203740_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203742_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203742_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203746_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203746_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:29.18 +14:24:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.825 3346876939268245376 088.62131814771 +14.41462458339 13.7117 13.2898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203750_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203750_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:01.97 +17:01:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.749 3369596839526811008 096.50838554566 +17.02746764185 13.6130 13.1678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203752_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203752_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:57.08 +12:23:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.432 3343070674829431296 089.23852167394 +12.38453820299 13.8070 13.3884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203762_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203762_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:24.02 +17:40:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203763_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203763_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203768_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203768_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:46.95 +13:55:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.890 3345330583541793152 090.69587578830 +13.92552475657 13.7644 13.2141 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 203769_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203769_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:45.29 +11:45:17.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 203770_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203770_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:45.90 +17:35:33.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 203775_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203775_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:19.43 +15:41:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.065 3348058776829742080 088.08070860564 +15.68555816579 13.4646 12.6353 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 203778_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203778_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:29.21 +14:44:35.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 203779_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203779_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:26.99 +13:56:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.022 3346656628923655296 087.36233592340 +13.93502683801 13.5841 12.9913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203789_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203789_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:26.75 +11:52:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 5.240 3342554041803119744 091.11160799284 +11.87555177583 13.7394 13.1750 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 203795_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203795_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:24.14 +14:13:42.6 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 203804_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203804_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:59.22 +11:22:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.754 3331028720404948736 097.24610593633 +11.36798480026 13.4467 12.8591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203811_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203811_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:54.93 +15:49:11.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)
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Considering the candidate 203813_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203813_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:19:42.85 +11:01:39.5 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 203818_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203818_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:43.11 +17:24:36.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)
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Considering the candidate 203819_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203819_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203821_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203821_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:19:54.85 +16:48:27.7 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 203829_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203829_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:33.49 +14:52:27.8 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 203835_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203835_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203840_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203840_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:23.90 +16:35:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.871 3349290813969029504 090.59953164843 +16.59742558105 13.6504 13.0447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203843_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203843_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203847_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203847_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:57.23 +14:11:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.685 3344605902299249664 094.23820934964 +14.18649888770 13.4499 12.5087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203851_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203851_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 203854_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203854_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203857_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203857_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203868_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203868_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203872_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203872_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:06:21.42 +11:26:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.867 3342293285749216768 091.58921954162 +11.43270391579 13.6667 13.1442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203873_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203873_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:12.20 +11:43:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203876_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203876_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:11.95 +12:16:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.108 3343378911745513600 089.79975530818 +12.27227598907 13.7335 13.3991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203877_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203877_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:18:12.86 +17:18:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.795 3370276131553875840 094.55312239852 +17.31028498507 13.3601 12.4758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203882_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203882_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203883_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203883_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:38.19 +17:10:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 5.041 3349816758482521344 089.15897259876 +17.18044062264 13.5462 12.7455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203887_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203887_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203888_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203888_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203898_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203898_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203901_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203901_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:56.74 +18:06:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.656 3350297386801211776 090.98632411144 +18.10023689286 13.6378 13.0475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203906_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203906_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:55.19 +10:09:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203921_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203921_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203932_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203932_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:24:00.44 +16:38:30.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 203938_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203938_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:17.94 +15:56:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203942_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203942_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203945_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203945_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:34.48 +13:53:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)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 203947_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203947_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203952_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203952_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:24:19.70 +15:59:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203954_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203954_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:26.75 +17:05:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203956_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203956_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:11.04 +12:04:06.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 203958_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203958_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:56.19 +14:18:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203959_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203959_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203963_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203963_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:21.91 +14:28:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.778 3346936592073193600 089.34178083077 +14.47459341375 13.4048 12.6377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203964_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203964_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203967_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203967_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:32.07 +13:11:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.224 3344141972817798528 093.13354346186 +13.19463435012 13.7028 13.1604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203968_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203968_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:48:08.73 +15:56:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 5.807 3348304040940723200 087.03646396936 +15.94438910480 13.5361 12.9408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203969_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 203969_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 203971_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203971_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:00.72 +17:02:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203979_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203979_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:50.74 +16:23:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.557 3369878482002662400 094.46182335388 +16.39774017797 13.6280 12.5970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203982_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203982_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:20.22 +16:40:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 5.381 3349341185345274240 090.33401976166 +16.66791045365 13.4465 12.4130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203993_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 203993_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:23:28.53 +14:14:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.034 3332644723322224512 095.86792216595 +14.24892112078 13.9313 13.3467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204000_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204000_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204009_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204009_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:29:39.20 +11:43:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.444 3331139015162664960 097.41324757429 +11.72494123221 13.4556 12.9486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.444#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_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204012_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:30.86 +15:57:22.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
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Considering the candidate 204013_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204013_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:02.07 +14:27:32.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 204021_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204021_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:03:25.40 +13:59:22.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 204023_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204023_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204025_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204025_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204027_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204027_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:30.18 +16:51:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 4.925 3349723613531441792 089.37560477446 +16.84980561661 14.2129 13.6865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204042_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204042_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204054_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204054_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:15.52 +10:20:58.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 204059_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204059_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:25:54.37 +17:17:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 5.108 3369658167363724928 096.47609072572 +17.29742569394 13.5208 13.1639 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 204066_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204066_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204068_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204068_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:24:23.56 +13:02:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.453 3332267285892796800 096.09763539836 +13.03365419127 13.6667 13.1735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204075_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204075_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204080_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204080_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204089_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204089_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:49.49 +12:58:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.339 3343527109594291712 090.70578778865 +12.98013013461 13.9841 13.4226 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 204093_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204093_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:36.56 +12:15:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.524 3331968115652147840 094.15247833434 +12.26200137289 13.3253 12.4223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204100_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204100_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:16.62 +11:26:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.231 3337084830447965568 087.31851523160 +11.43854329547 14.0273 13.4622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204101_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204101_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:44.06 +15:24:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204102_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204102_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:53.53 +13:39:17.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)
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Considering the candidate 204113_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204113_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:14:14.25 +13:14:58.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)
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Considering the candidate 204121_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204121_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204127_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204127_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:46.73 +15:24:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 5.852 3348015762736196224 088.19464392083 +15.39901443330 13.5331 12.7649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204139_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204139_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204147_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204147_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204158_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204158_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204159_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204159_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204160_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204160_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204166_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204166_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:22:17.46 +14:41:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.209 3368700290873546368 095.57303977842 +14.68726504898 13.6776 13.1286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204178_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204178_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204179_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204179_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204180_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204180_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:42.58 +18:05:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.617 3371314100594722048 097.17742183438 +18.09499536501 13.7279 13.1675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204184_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204184_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204186_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204186_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204188_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204188_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:32.65 +17:42:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 5.049 3350213961356368256 089.63560695884 +17.70863236355 13.4533 12.4621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204198_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204198_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:34:03.50 +17:03:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.593 3370946593129054208 098.51442328124 +17.05109453628 13.4551 12.5253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204199_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204199_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:07:29.86 +09:59:20.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 204202_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204202_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204207_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204207_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204216_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204216_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204220_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204220_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:19.25 +11:24:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.804 3342280813164107904 092.08007562927 +11.41108871148 13.8708 13.5181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204224_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204224_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204225_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204225_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:57.03 +12:14:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.718 3343051089778622464 089.23769903909 +12.24546925573 13.8166 13.2858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204231_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204231_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:56.18 +17:30:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.909 3369755409718775040 096.73359389243 +17.50577421651 13.8902 13.2695 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 204233_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204233_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204241_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204241_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204243_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204243_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:15.92 +15:25:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.813 3348602283468997504 091.06602424260 +15.41561331360 14.0165 13.4935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204246_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204246_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204249_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204249_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204258_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204258_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:49:52.98 +13:28:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 5.385 3346419993405922688 087.47086539119 +13.46842504712 13.7153 12.9254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204265_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204265_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204273_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204273_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204284_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204284_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204287_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204287_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:19:07.06 +18:17:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 4.653 3370749467012738048 094.77996768169 +18.28748482244 13.0059 11.7675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204303_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204303_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:50:48.56 +15:39:14.7 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 204304_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204304_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204307_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204307_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204308_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204308_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204324_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204324_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:28.52 +14:16:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 5.351 3344804089271135360 093.86789478730 +14.27957439078 14.1119 13.5959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204328_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204328_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:07.74 +17:00:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 4.774 3349744637392153600 089.78210980170 +16.99929178639 13.3151 12.2317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204335_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204335_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:28:32.32 +13:51:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204337_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204337_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:17:58.48 +13:20:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.563 3332480488069592064 094.49408703400 +13.33407798648 14.1866 13.4502 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#
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Considering the candidate 204341_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204341_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204343_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204343_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204348_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204348_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:31.83 +11:59:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 5.183 3342995152124616320 089.38246282233 +11.99445805621 13.9131 13.3876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204354_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204354_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:16.94 +17:47:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204359_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204359_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204362_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204362_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:38.72 +14:50:44.0 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 204364_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204364_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:26.90 +12:46:37.4 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 204371_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204371_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:09:57.08 +16:59:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 5.711 3349191724779334272 092.48815809744 +16.98505547169 13.7776 13.0511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204372_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204372_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:05.70 +14:12:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 5.576 3343914172047013248 090.02347495254 +14.21289096570 13.9893 13.6189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204373_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204373_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204377_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204377_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:01:00.86 +18:02:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.263 3350331162424218368 090.25327253217 +18.03384602834 13.8045 13.3758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204378_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204378_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:14.52 +14:14:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 4.790 3343912969456198016 089.81062497295 +14.23886949336 13.7699 13.2598 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 204386_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204386_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204399_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204399_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204413_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204413_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204419_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204419_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204421_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204421_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:18:17.44 +12:04:28.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 204422_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204422_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204427_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204427_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:09.95 +16:18:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 5.303 3348939077624336256 089.54108338839 +16.31093257125 14.1595 13.5756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204430_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204430_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204459_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204459_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204460_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204460_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204464_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204464_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204465_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204465_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204467_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204467_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204478_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204478_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204493_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204493_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:24:16.64 +17:01:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 4.339 3369622609330283520 096.06860895783 +17.01768013797 14.1065 13.4636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204498_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204498_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204499_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204499_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:46.10 +16:16:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 5.832 3349598475364583424 089.19279665427 +16.27986520680 14.0892 13.5796 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 204508_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204508_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204510_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204510_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204522_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204522_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:43.20 +17:27:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204526_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204526_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:56:31.98 +17:39:22.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)
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Considering the candidate 204528_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204528_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204547_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204547_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204555_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204555_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204565_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204565_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:20.21 +13:53:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 3.367 3343829715810741760 090.58416012908 +13.88370487902 14.4205 13.8796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204572_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204572_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204576_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204576_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:00:39.01 +10:32:24.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 204581_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204581_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204582_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204582_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:54:43.28 +10:26:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.588 3336019438039885952 088.67973659359 +10.44011868399 13.7016 12.8863 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#
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Considering the candidate 204583_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204583_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204589_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204589_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204593_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204593_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:23.67 +14:28:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 4.509 3346936695152404480 089.34925582038 +14.48032327888 13.6926 13.1660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204600_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204600_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:56.16 +18:10:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 4.071 3373570268389083520 091.48383793674 +18.17418525058 14.0389 13.5085 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#
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Considering the candidate 204602_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204602_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204605_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204605_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204618_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204618_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204629_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204629_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204634_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204634_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:19:17.36 +13:05:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 4.360 3332414306914764160 094.82223529244 +13.09459823887 14.1217 13.5750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204638_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204638_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204641_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204641_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204642_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204642_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204650_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204650_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:43.47 +15:55:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 5.720 3348823250946936704 089.43132091629 +15.91792230642 14.0093 13.5216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204657_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204657_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204666_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204666_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204686_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204686_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204687_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204687_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:06.45 +11:12:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 5.533 3330299194438996096 092.77642022600 +11.21444593758 14.0752 13.6558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204691_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204691_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:16:48.85 +15:29:12.5 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 204692_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204692_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204693_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204693_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:32.15 +13:55:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 5.502 3345190185354113792 092.13406987695 +13.92805890460 13.6268 12.6096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204697_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204697_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:00.52 +16:15:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.875 3349606240665661056 088.75212541171 +16.25120202087 14.1899 13.6350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204705_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204705_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:13:54.34 +17:32:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 5.754 3370240431785028864 093.47626053637 +17.54568642566 13.1651 11.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204715_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204715_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204722_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204722_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204745_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204745_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:26:48.61 +18:03:52.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)
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Considering the candidate 204750_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204750_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204760_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204760_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:57:20.30 +11:45:12.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)
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Considering the candidate 204765_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204765_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:20:31.02 +13:22:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 5.589 3332443448271854208 095.12857093767 +13.37048385213 14.1817 13.5525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204787_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204787_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204810_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204810_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204815_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204815_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:10.82 +14:43:50.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 204820_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204820_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:41:03.05 +14:43:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.975 3355989558499299200 100.26235070860 +14.71566214103 14.0197 13.5080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204839_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204839_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204852_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204852_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:14.52 +15:02:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204853_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204853_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204857_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204857_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 204858_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204858_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204868_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204868_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204874_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204874_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:38.62 +14:21:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 5.174 3345361953982546560 090.66096814153 +14.36025821167 13.9148 13.2457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204878_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204878_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204879_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204879_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204910_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204910_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204939_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204939_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:07.23 +15:07:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204958_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204958_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:05:20.06 +13:46:20.8 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 204968_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204968_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:06.12 +16:09:28.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204984_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204984_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204985_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 204985_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204998_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 204998_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:11:27.69 +11:53:58.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)
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Considering the candidate 205001_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205001_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205003_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205003_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205005_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205005_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:49.25 +15:12:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 5.072 3347223117931582080 088.95540874545 +15.21332663890 14.1250 13.7022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205014_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205014_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205061_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205061_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205065_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205065_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205072_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205072_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205076_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205076_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205083_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205083_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205086_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205086_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205092_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205092_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:30.39 +17:44:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 5.013 3350217122452294912 089.62654034884 +17.74488772580 14.1234 13.5710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205105_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205105_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205111_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205111_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205113_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205113_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205121_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205121_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:46.83 +16:37:26.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)
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Considering the candidate 205130_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205130_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205136_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205136_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205149_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205149_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205161_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205161_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:37:20.27 +13:51:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 5.772 3355836279706743680 099.33339413383 +13.86266276783 14.2105 13.6895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205167_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205167_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205174_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205174_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205179_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205179_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:42:13.80 +17:53:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 5.581 3359418488590430976 100.55776283494 +17.88899778679 14.3955 13.6766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205180_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205180_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205188_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205188_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:55:19.81 +11:39:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 4.076 3342911967197644800 088.83263984573 +11.65573293740 14.0060 13.2508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205194_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205194_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205204_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205204_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205205_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205205_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205210_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205210_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:52:20.65 +15:43:32.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
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Considering the candidate 205214_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205214_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205216_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205216_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205222_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205222_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:10:34.02 +12:23:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 4.828 3343947432273696128 092.64208448727 +12.39308825072 14.5242 13.9399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205224_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205224_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205231_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205231_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205235_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205235_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205236_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205236_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205242_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205242_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205243_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205243_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205255_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205255_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205266_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205266_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205269_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205269_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:57.60 +13:40:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205274_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205274_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:07.92 +11:38:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 4.474 3342947117210858496 089.53308816318 +11.64739898364 14.3631 13.9011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205277_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205277_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205291_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205291_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 205302_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205302_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205305_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205305_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:15:45.25 +12:01:05.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)
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Considering the candidate 205306_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205306_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:32.65 +13:11:25.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)
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Considering the candidate 205312_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205312_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205322_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205322_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205327_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205327_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205342_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205342_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205344_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205344_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:04:16.28 +12:46:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205348_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205348_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205351_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205351_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205356_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205356_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205363_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205363_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205370_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205370_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205371_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205371_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205379_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205379_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205405_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205405_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205407_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205407_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205408_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205408_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205417_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205417_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205419_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205419_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:21:08.36 +15:57:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 4.238 3369043849598977920 095.28399210695 +15.95920019651 14.7804 14.2242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205421_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205421_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205425_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205425_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:59:04.92 +14:59:47.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)
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Considering the candidate 205428_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205428_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 205431_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205431_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205444_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205444_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205446_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205446_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205447_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205447_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205449_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205449_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205451_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205451_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205453_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205453_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205461_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205461_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205467_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205467_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205470_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205470_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205476_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205476_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205493_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205493_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205499_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205499_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205505_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205505_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205506_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205506_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205508_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205508_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205511_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205511_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205527_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205527_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205540_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205540_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:08:56.15 +10:08:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 5.590 3329938520264483328 092.23358785827 +10.13926830152 14.4563 13.9127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205567_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205567_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205568_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205568_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205578_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205578_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205584_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205584_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205602_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205602_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205603_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205603_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205609_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205609_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205617_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205617_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205635_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205635_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205644_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205644_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205653_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 205653_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 205658_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205658_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 05:58:08.88 +13:48:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 5.251 3343870947496327680 089.53717199221 +13.80343986307 14.3430 13.6111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205667_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205667_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:02:58.30 +10:30:08.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)
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Considering the candidate 205686_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
The candidate 205686_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 06:12:09.75 +13:57:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124797_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 124797_fd_Ori-02-Q2b1x1_2026-03-28_21-57-36_20.00sec_-15.00C_LIGHT_0060
make_report_in_HTML.sh Phase 2 (HTML assembly): 73s
make_report_in_HTML.sh TOTAL: 800s
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 ####
06:35:44.94 +11:17:01.3
05:58:23.77 +11:50:43.6
06:17:32.29 +16:47:23.0
06:02:38.33 +14:07:59.3
06:16:41.50 +14:25:10.4
06:15:49.41 +13:13:07.8
06:19:01.55 +14:21:47.0
05:54:48.72 +13:47:50.8
06:25:19.99 +15:08:17.2
06:16:49.33 +14:56:25.0
06:12:29.71 +12:51:00.4
06:08:08.32 +14:27:06.1
06:20:10.22 +12:07:10.0
06:04:08.81 +11:12:57.6
06:03:03.62 +13:25:03.3
06:07:50.05 +12:50:04.1
05:57:25.12 +15:34:07.5
05:58:51.50 +15:39:36.4
06:28:32.96 +15:25:10.6
05:50:29.23 +15:16:05.2
05:51:58.05 +15:48:26.5
05:55:21.81 +15:39:09.6
06:36:29.76 +16:46:34.6
06:21:43.51 +12:44:21.3
06:08:07.79 +15:55:02.4
06:07:08.77 +12:32:29.9
05:51:07.57 +10:13:07.3
06:20:58.24 +16:02:33.0
05:56:05.78 +17:53:51.3
05:57:50.52 +15:53:33.9
06:35:48.68 +18:02:11.9
06:35:19.20 +14:30:00.3
06:07:05.41 +10:57:47.1
05:52:23.96 +13:19:35.4
06:13:51.21 +16:29:05.2
06:00:30.08 +09:53:10.7
06:18:53.63 +17:20:32.0
06:41:08.40 +16:06:36.5
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06:10:22.30 +16:14:32.0
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06:28:49.44 +15:22:57.9
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06:01:20.73 +13:05:22.2
06:13:39.34 +15:30:56.7
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05:55:30.14 +15:07:44.4
06:15:20.07 +14:59:21.8
05:53:57.36 +12:16:41.1
05:50:05.30 +10:34:52.5
06:02:09.71 +12:11:04.8
06:27:07.95 +16:55:01.9
05:58:18.72 +18:08:55.4
05:53:22.72 +12:06:18.0
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06:20:46.12 +17:46:19.4
06:10:32.47 +16:29:30.3
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05:55:47.09 +14:33:50.9
06:00:25.20 +16:41:37.4
06:27:09.44 +15:25:23.6
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06:32:06.11 +18:09:37.2
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05:57:25.91 +11:32:51.5
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06:39:55.14 +13:35:03.6
06:01:02.76 +13:48:59.6
06:35:42.69 +11:30:05.7
06:41:18.50 +18:02:07.2
05:49:55.21 +12:51:44.4
06:31:42.82 +11:11:14.9
06:36:11.37 +17:16:23.4
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06:25:55.13 +15:51:16.3
06:40:48.75 +17:56:48.8
06:26:36.81 +17:47:21.7
05:49:25.37 +10:51:15.1
05:50:34.10 +14:49:09.8
06:41:51.58 +15:27:19.7
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05:56:53.26 +14:50:24.2
06:16:27.36 +16:42:37.2
06:03:45.61 +14:20:46.4
06:30:33.66 +17:55:15.4
06:16:45.41 +15:33:25.8
06:10:12.01 +17:42:33.7
06:23:25.04 +17:30:59.4
06:19:42.39 +15:59:26.3
06:11:37.59 +13:51:44.9
06:08:41.20 +17:23:37.2
06:13:09.91 +18:03:25.5
06:05:30.91 +16:17:58.0
05:57:13.90 +17:30:31.9
06:10:33.18 +17:47:20.1
05:57:47.60 +14:19:57.4
06:17:11.15 +15:50:14.3
05:56:44.14 +17:00:11.1
06:18:18.15 +14:22:19.4
06:16:56.03 +15:17:01.8
06:10:55.69 +15:29:38.5
06:09:52.24 +11:19:55.0
06:35:06.77 +12:37:58.3
06:37:54.50 +17:30:25.6
06:20:46.44 +15:18:14.8
06:22:11.62 +16:05:21.3
05:56:26.65 +17:40:49.6
06:25:09.44 +15:58:53.2
06:07:01.07 +10:58:45.5
06:10:14.13 +13:48:21.8
06:02:06.73 +15:11:09.4
06:12:57.12 +17:26:20.6
06:17:52.61 +15:42:08.3
05:57:12.71 +17:39:14.8
06:27:55.34 +17:41:36.1
06:06:27.04 +10:44:01.4
06:10:30.91 +14:52:41.1
06:12:28.10 +15:20:03.5
06:29:40.10 +11:43:01.9
06:07:20.22 +16:45:35.4
06:14:37.25 +16:02:29.7
06:38:54.79 +15:11:20.6
05:54:13.85 +13:11:37.5
06:35:02.86 +17:42:00.9
05:56:33.25 +15:11:30.2
06:22:05.27 +17:47:57.3
06:27:44.25 +17:39:43.5
06:19:14.38 +17:25:24.8
06:16:19.85 +14:31:16.3
05:54:35.46 +12:10:02.2
06:00:20.47 +15:32:27.5
05:59:54.86 +17:17:28.4
06:14:42.27 +15:10:59.5
05:58:48.35 +13:38:11.6
05:57:00.05 +17:55:40.0
06:34:47.09 +15:31:01.1
06:15:28.00 +14:23:53.4
05:54:30.48 +12:57:30.9
06:20:57.18 +16:50:14.0
06:31:32.15 +18:03:36.5
06:11:37.15 +15:28:26.2
05:54:22.03 +15:30:54.7
05:49:14.20 +14:41:49.7
05:58:26.34 +15:59:27.6
06:19:47.07 +16:38:51.9
05:57:13.12 +12:48:33.4
06:06:58.48 +14:36:07.9
06:12:31.18 +15:20:12.7
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06:18:54.41 +11:33:57.4
06:21:38.01 +12:02:48.8
05:49:28.23 +11:30:41.3
06:12:26.70 +15:00:24.4
06:02:32.64 +14:05:00.5
06:04:53.18 +10:54:04.3
05:57:33.73 +15:38:38.1
06:10:46.67 +14:47:19.1
05:48:53.22 +10:13:09.7
05:56:30.04 +12:01:33.2
06:07:36.39 +10:59:23.3
05:50:55.72 +13:52:50.5
06:19:12.12 +12:45:05.8
06:41:44.73 +15:13:17.5
06:23:49.23 +16:28:13.4
06:11:05.87 +16:19:10.2
05:50:50.16 +14:25:32.6
06:01:37.66 +14:43:11.3
05:55:56.95 +15:40:28.5
05:56:21.65 +17:58:16.6
06:20:58.57 +14:41:22.8
05:58:16.45 +16:05:42.7
05:48:53.57 +10:23:25.0
05:58:03.65 +15:30:43.4
06:26:05.78 +16:32:36.8
06:18:06.36 +11:26:20.6
06:25:59.18 +14:56:44.5
06:12:49.42 +11:40:07.8
06:09:15.54 +11:12:53.5
06:05:26.55 +12:45:45.3
06:00:57.42 +16:27:52.8
05:57:34.57 +11:12:21.5
06:11:09.02 +17:31:04.6
06:13:14.11 +13:29:52.0
05:50:37.80 +12:00:50.3
06:28:04.93 +14:04:45.4
05:51:00.49 +13:29:08.0
06:19:04.28 +16:47:19.9
06:05:37.30 +17:10:43.6
05:53:09.28 +11:49:52.4
06:14:02.40 +15:01:15.6
06:29:32.69 +17:39:52.8
05:50:32.94 +15:45:58.9
06:12:18.19 +15:12:21.7
06:13:16.49 +15:43:24.4
06:25:40.26 +17:47:38.4
06:09:55.66 +14:26:06.5
06:01:34.55 +16:08:07.9
06:02:46.01 +11:05:17.8
05:59:14.13 +16:16:41.1
06:19:02.10 +16:47:08.2
05:51:57.97 +14:40:17.5
05:50:16.03 +13:54:05.4
05:53:56.26 +15:51:26.8
06:27:51.81 +16:41:07.0
05:53:13.27 +14:40:26.4
05:51:52.97 +15:55:28.7
06:16:58.71 +18:09:12.0
06:17:35.48 +14:21:38.5
06:26:03.55 +16:32:25.5
06:01:33.58 +16:49:51.0
06:18:42.38 +17:53:59.0
06:20:51.87 +17:05:08.9
05:52:58.21 +15:17:40.7
06:06:48.58 +16:40:37.3
06:11:58.99 +17:22:43.8
05:56:29.76 +15:23:10.1
06:14:08.37 +17:22:59.0
05:56:56.29 +16:55:37.5
05:59:56.14 +11:30:33.4
06:01:42.15 +16:14:30.0
05:55:47.25 +14:48:04.2
06:14:35.32 +13:49:52.5
06:18:28.87 +14:20:26.5
06:06:22.14 +14:21:40.1
06:00:22.07 +10:05:27.1
06:18:52.50 +13:48:26.1
06:05:27.21 +10:56:04.5
06:11:38.95 +16:33:10.4
06:39:09.96 +13:11:14.6
06:01:17.73 +15:06:07.6
06:16:11.26 +14:06:20.4
06:08:55.85 +17:07:40.2
06:01:32.33 +14:49:01.0
06:15:38.04 +17:53:12.8
05:58:07.88 +17:09:02.1
06:10:40.74 +15:14:02.4
06:25:33.70 +17:35:15.0
06:01:19.57 +15:34:36.3
06:12:51.31 +13:17:02.7
06:39:17.07 +15:47:13.6
05:52:24.03 +13:07:42.6
06:36:16.00 +17:59:28.7
06:20:14.51 +13:20:23.6
06:13:50.87 +14:44:31.4
06:16:27.29 +14:57:43.4
05:49:53.48 +12:29:46.2
06:06:01.07 +16:53:34.0
06:14:07.62 +18:00:35.3
06:15:51.77 +13:13:57.6
06:04:27.92 +16:29:13.6
05:52:31.28 +12:19:33.1
05:55:56.68 +14:38:13.5
06:10:29.67 +16:02:29.5
05:50:03.82 +10:24:32.0
06:17:27.92 +11:05:42.8
06:10:25.17 +16:38:52.0
06:20:25.62 +16:52:34.9
05:58:52.31 +13:37:23.5
06:25:04.28 +16:36:40.6
05:49:46.29 +14:47:43.5
06:07:09.47 +16:42:47.4
05:58:56.45 +18:06:46.5
05:59:52.66 +12:19:21.9
06:06:04.83 +13:40:16.8
06:11:18.41 +14:47:53.9
05:56:54.46 +15:03:06.2
06:27:52.40 +16:41:35.9
06:25:51.85 +15:01:10.9
05:58:27.90 +15:59:40.8
05:48:20.40 +13:06:39.3
06:10:34.15 +18:09:01.8
06:38:54.23 +17:47:26.8
06:27:31.24 +15:16:12.7
05:52:03.71 +15:17:56.9
05:49:09.18 +15:28:21.4
06:11:39.60 +16:27:38.5
05:58:55.65 +14:23:33.8
06:19:36.65 +17:40:28.7
06:10:28.05 +13:50:01.6
05:55:50.17 +17:41:15.7
05:49:45.62 +14:44:54.6
05:57:35.77 +15:03:49.6
05:59:50.35 +16:54:20.2
05:58:04.82 +13:32:09.6
05:57:41.34 +17:40:40.5
06:01:56.65 +16:44:38.7
05:50:36.42 +14:31:42.7
06:00:53.07 +12:13:41.6
06:06:05.08 +13:21:02.4
06:00:38.99 +15:55:36.4
05:56:38.86 +17:44:21.4
06:19:59.31 +17:10:05.9
05:54:24.85 +15:55:48.1
05:56:30.45 +15:24:06.3
05:58:28.09 +17:33:01.5
05:53:45.27 +15:46:35.8
06:00:54.64 +15:22:19.2
06:15:24.32 +13:24:20.3
05:59:39.43 +13:09:23.1
06:01:32.19 +16:40:16.4
06:10:33.47 +16:28:35.0
05:48:48.99 +15:03:36.3
05:56:31.53 +16:33:11.6
06:02:07.05 +16:19:41.2
06:08:01.86 +15:33:58.0
05:50:06.04 +12:53:14.1
05:52:28.71 +14:24:30.1
06:01:17.11 +15:30:04.1
05:55:42.04 +14:41:21.9
05:58:42.60 +11:51:00.9
05:58:09.45 +17:20:40.6
06:02:05.99 +16:03:13.3
06:10:07.81 +15:00:28.2
05:52:47.63 +15:52:24.7
05:53:45.05 +15:09:38.0
05:53:06.34 +14:57:36.0
05:51:06.34 +15:03:05.9
05:51:24.40 +15:08:08.5
05:54:14.08 +15:13:42.7
06:04:04.16 +17:40:32.2
06:20:00.56 +17:12:18.2
05:57:32.63 +14:41:17.1
05:54:08.57 +14:53:55.7
05:57:11.85 +14:38:51.9
06:02:12.90 +14:59:52.0
06:06:52.06 +15:48:39.0
05:56:30.91 +12:09:19.9
06:03:42.69 +13:07:00.2
########### 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 ####
06:35:44.94 +11:17:01.3
06:17:32.29 +16:47:23.0
06:02:38.33 +14:07:59.3
06:16:41.50 +14:25:10.4
06:15:49.41 +13:13:07.8
06:19:01.55 +14:21:47.0
05:54:48.72 +13:47:50.8
06:25:19.99 +15:08:17.2
06:16:49.33 +14:56:25.0
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06:20:10.22 +12:07:10.0
06:04:08.81 +11:12:57.6
06:03:03.62 +13:25:03.3
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05:57:25.12 +15:34:07.5
05:58:51.50 +15:39:36.4
06:28:32.96 +15:25:10.6
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05:51:58.05 +15:48:26.5
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05:56:05.78 +17:53:51.3
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05:52:23.96 +13:19:35.4
06:13:51.21 +16:29:05.2
06:00:30.08 +09:53:10.7
06:18:53.63 +17:20:32.0
06:41:08.40 +16:06:36.5
05:53:16.81 +14:42:25.5
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05:55:49.49 +17:04:43.7
06:26:09.52 +14:11:10.7
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06:20:06.66 +15:51:59.5
06:15:50.93 +17:58:53.9
06:21:19.04 +12:51:49.2
06:28:49.44 +15:22:57.9
06:25:36.63 +13:37:49.9
06:01:20.73 +13:05:22.2
06:13:39.34 +15:30:56.7
06:06:13.05 +16:19:25.1
05:57:00.14 +13:28:56.4
06:02:12.33 +12:06:05.4
05:55:30.14 +15:07:44.4
06:15:20.07 +14:59:21.8
05:53:57.36 +12:16:41.1
05:50:05.30 +10:34:52.5
06:02:09.71 +12:11:04.8
06:27:07.95 +16:55:01.9
05:58:18.72 +18:08:55.4
05:53:22.72 +12:06:18.0
05:57:16.62 +12:53:47.2
06:20:46.12 +17:46:19.4
06:10:32.47 +16:29:30.3
05:59:16.87 +12:05:09.6
05:51:37.51 +13:14:02.5
06:12:20.10 +10:02:03.9
05:53:57.38 +15:58:38.5
06:10:55.23 +18:14:13.8
05:58:27.39 +16:42:25.2
05:54:00.73 +14:50:42.4
06:34:16.98 +17:15:29.9
06:13:58.17 +14:27:25.2
06:13:27.44 +14:13:52.4
06:13:55.42 +12:05:34.8
06:29:40.32 +17:17:01.6
05:52:18.18 +15:51:58.7
06:02:24.65 +14:17:47.4
06:24:13.84 +15:54:30.3
06:18:02.62 +17:41:17.8
06:38:34.20 +17:37:22.6
05:54:41.60 +12:22:48.9
06:11:23.67 +14:49:43.7
06:15:53.67 +14:10:16.5
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05:55:31.07 +15:11:03.3
06:09:12.84 +15:40:25.5
05:51:38.55 +14:47:55.2
06:13:23.68 +17:13:26.6
05:51:05.88 +15:39:53.7
06:00:53.36 +14:53:46.9
05:55:47.09 +14:33:50.9
06:00:25.20 +16:41:37.4
06:27:09.44 +15:25:23.6
06:38:45.68 +13:41:32.4
06:32:06.11 +18:09:37.2
06:13:48.73 +12:57:35.1
05:57:25.91 +11:32:51.5
06:14:38.16 +13:49:46.1
06:39:55.14 +13:35:03.6
06:01:02.76 +13:48:59.6
06:35:42.69 +11:30:05.7
06:41:18.50 +18:02:07.2
05:49:55.21 +12:51:44.4
06:31:42.82 +11:11:14.9
06:36:11.37 +17:16:23.4
05:55:57.28 +16:32:15.5
06:25:55.13 +15:51:16.3
06:40:48.75 +17:56:48.8
06:26:36.81 +17:47:21.7
05:49:25.37 +10:51:15.1
05:50:34.10 +14:49:09.8
06:41:51.58 +15:27:19.7
06:06:26.73 +10:44:52.7
05:56:53.26 +14:50:24.2
06:16:27.36 +16:42:37.2
06:03:45.61 +14:20:46.4
06:30:33.66 +17:55:15.4
06:16:45.41 +15:33:25.8
06:10:12.01 +17:42:33.7
06:23:25.04 +17:30:59.4
06:19:42.39 +15:59:26.3
06:11:37.59 +13:51:44.9
06:08:41.20 +17:23:37.2
06:13:09.91 +18:03:25.5
06:05:30.91 +16:17:58.0
05:57:13.90 +17:30:31.9
06:10:33.18 +17:47:20.1
05:57:47.60 +14:19:57.4
06:17:11.15 +15:50:14.3
05:56:44.14 +17:00:11.1
06:18:18.15 +14:22:19.4
06:16:56.03 +15:17:01.8
06:10:55.69 +15:29:38.5
06:09:52.24 +11:19:55.0
06:35:06.77 +12:37:58.3
06:37:54.50 +17:30:25.6
06:20:46.44 +15:18:14.8
06:22:11.62 +16:05:21.3
05:56:26.65 +17:40:49.6
06:25:09.44 +15:58:53.2
06:07:01.07 +10:58:45.5
06:10:14.13 +13:48:21.8
06:02:06.73 +15:11:09.4
06:12:57.12 +17:26:20.6
06:17:52.61 +15:42:08.3
05:57:12.71 +17:39:14.8
06:27:55.34 +17:41:36.1
06:06:27.04 +10:44:01.4
06:10:30.91 +14:52:41.1
06:12:28.10 +15:20:03.5
06:29:40.10 +11:43:01.9
06:07:20.22 +16:45:35.4
06:14:37.25 +16:02:29.7
06:38:54.79 +15:11:20.6
05:54:13.85 +13:11:37.5
06:35:02.86 +17:42:00.9
05:56:33.25 +15:11:30.2
06:22:05.27 +17:47:57.3
06:27:44.25 +17:39:43.5
06:19:14.38 +17:25:24.8
06:16:19.85 +14:31:16.3
05:54:35.46 +12:10:02.2
06:00:20.47 +15:32:27.5
05:59:54.86 +17:17:28.4
06:14:42.27 +15:10:59.5
05:58:48.35 +13:38:11.6
05:57:00.05 +17:55:40.0
06:34:47.09 +15:31:01.1
06:15:28.00 +14:23:53.4
05:54:30.48 +12:57:30.9
06:20:57.18 +16:50:14.0
06:31:32.15 +18:03:36.5
06:11:37.15 +15:28:26.2
05:54:22.03 +15:30:54.7
05:49:14.20 +14:41:49.7
05:58:26.34 +15:59:27.6
06:19:47.07 +16:38:51.9
05:57:13.12 +12:48:33.4
06:06:58.48 +14:36:07.9
06:12:31.18 +15:20:12.7
06:03:52.36 +14:59:05.9
06:18:54.41 +11:33:57.4
06:21:38.01 +12:02:48.8
05:49:28.23 +11:30:41.3
06:12:26.70 +15:00:24.4
06:02:32.64 +14:05:00.5
06:04:53.18 +10:54:04.3
05:57:33.73 +15:38:38.1
06:10:46.67 +14:47:19.1
05:48:53.22 +10:13:09.7
05:56:30.04 +12:01:33.2
06:07:36.39 +10:59:23.3
05:50:55.72 +13:52:50.5
06:19:12.12 +12:45:05.8
06:41:44.73 +15:13:17.5
06:23:49.23 +16:28:13.4
06:11:05.87 +16:19:10.2
05:50:50.16 +14:25:32.6
06:01:37.66 +14:43:11.3
05:55:56.95 +15:40:28.5
05:56:21.65 +17:58:16.6
06:20:58.57 +14:41:22.8
05:58:16.45 +16:05:42.7
05:48:53.57 +10:23:25.0
05:58:03.65 +15:30:43.4
06:26:05.78 +16:32:36.8
06:18:06.36 +11:26:20.6
06:25:59.18 +14:56:44.5
06:12:49.42 +11:40:07.8
06:09:15.54 +11:12:53.5
06:05:26.55 +12:45:45.3
06:00:57.42 +16:27:52.8
05:57:34.57 +11:12:21.5
06:11:09.02 +17:31:04.6
06:13:14.11 +13:29:52.0
05:50:37.80 +12:00:50.3
06:28:04.93 +14:04:45.4
05:51:00.49 +13:29:08.0
06:19:04.28 +16:47:19.9
06:05:37.30 +17:10:43.6
05:53:09.28 +11:49:52.4
06:14:02.40 +15:01:15.6
06:29:32.69 +17:39:52.8
05:50:32.94 +15:45:58.9
06:12:18.19 +15:12:21.7
06:13:16.49 +15:43:24.4
06:25:40.26 +17:47:38.4
06:09:55.66 +14:26:06.5
06:01:34.55 +16:08:07.9
06:02:46.01 +11:05:17.8
05:59:14.13 +16:16:41.1
06:19:02.10 +16:47:08.2
05:51:57.97 +14:40:17.5
05:50:16.03 +13:54:05.4
05:53:56.26 +15:51:26.8
06:27:51.81 +16:41:07.0
05:53:13.27 +14:40:26.4
05:51:52.97 +15:55:28.7
06:16:58.71 +18:09:12.0
06:17:35.48 +14:21:38.5
06:26:03.55 +16:32:25.5
06:01:33.58 +16:49:51.0
06:18:42.38 +17:53:59.0
06:20:51.87 +17:05:08.9
05:52:58.21 +15:17:40.7
06:06:48.58 +16:40:37.3
06:11:58.99 +17:22:43.8
05:56:29.76 +15:23:10.1
06:14:08.37 +17:22:59.0
05:56:56.29 +16:55:37.5
05:59:56.14 +11:30:33.4
06:01:42.15 +16:14:30.0
05:55:47.25 +14:48:04.2
06:14:35.32 +13:49:52.5
06:18:28.87 +14:20:26.5
06:06:22.14 +14:21:40.1
06:00:22.07 +10:05:27.1
06:18:52.50 +13:48:26.1
06:05:27.21 +10:56:04.5
06:11:38.95 +16:33:10.4
06:39:09.96 +13:11:14.6
06:01:17.73 +15:06:07.6
06:16:11.26 +14:06:20.4
06:08:55.85 +17:07:40.2
06:01:32.33 +14:49:01.0
06:15:38.04 +17:53:12.8
05:58:07.88 +17:09:02.1
06:10:40.74 +15:14:02.4
06:25:33.70 +17:35:15.0
06:01:19.57 +15:34:36.3
06:12:51.31 +13:17:02.7
06:39:17.07 +15:47:13.6
05:52:24.03 +13:07:42.6
06:36:16.00 +17:59:28.7
06:20:14.51 +13:20:23.6
06:13:50.87 +14:44:31.4
06:16:27.29 +14:57:43.4
05:49:53.48 +12:29:46.2
06:06:01.07 +16:53:34.0
06:14:07.62 +18:00:35.3
06:15:51.77 +13:13:57.6
06:04:27.92 +16:29:13.6
05:52:31.28 +12:19:33.1
05:55:56.68 +14:38:13.5
06:10:29.67 +16:02:29.5
05:50:03.82 +10:24:32.0
06:17:27.92 +11:05:42.8
06:10:25.17 +16:38:52.0
06:20:25.62 +16:52:34.9
05:58:52.31 +13:37:23.5
06:25:04.28 +16:36:40.6
05:49:46.29 +14:47:43.5
06:07:09.47 +16:42:47.4
05:58:56.45 +18:06:46.5
05:59:52.66 +12:19:21.9
06:06:04.83 +13:40:16.8
06:11:18.41 +14:47:53.9
05:56:54.46 +15:03:06.2
06:27:52.40 +16:41:35.9
06:25:51.85 +15:01:10.9
05:58:27.90 +15:59:40.8
05:48:20.40 +13:06:39.3
06:10:34.15 +18:09:01.8
06:38:54.23 +17:47:26.8
06:27:31.24 +15:16:12.7
05:52:03.71 +15:17:56.9
05:49:09.18 +15:28:21.4
06:11:39.60 +16:27:38.5
05:58:55.65 +14:23:33.8
06:19:36.65 +17:40:28.7
06:10:28.05 +13:50:01.6
05:55:50.17 +17:41:15.7
05:49:45.62 +14:44:54.6
05:57:35.77 +15:03:49.6
05:59:50.35 +16:54:20.2
05:58:04.82 +13:32:09.6
05:57:41.34 +17:40:40.5
06:01:56.65 +16:44:38.7
05:50:36.42 +14:31:42.7
06:00:53.07 +12:13:41.6
06:06:05.08 +13:21:02.4
06:00:38.99 +15:55:36.4
05:56:38.86 +17:44:21.4
06:19:59.31 +17:10:05.9
05:54:24.85 +15:55:48.1
05:56:30.45 +15:24:06.3
05:58:28.09 +17:33:01.5
05:53:45.27 +15:46:35.8
06:00:54.64 +15:22:19.2
06:15:24.32 +13:24:20.3
05:59:39.43 +13:09:23.1
06:01:32.19 +16:40:16.4
06:10:33.47 +16:28:35.0
05:48:48.99 +15:03:36.3
05:56:31.53 +16:33:11.6
06:02:07.05 +16:19:41.2
06:08:01.86 +15:33:58.0
05:50:06.04 +12:53:14.1
05:52:28.71 +14:24:30.1
06:01:17.11 +15:30:04.1
05:55:42.04 +14:41:21.9
05:58:42.60 +11:51:00.9
05:58:09.45 +17:20:40.6
06:02:05.99 +16:03:13.3
06:10:07.81 +15:00:28.2
05:52:47.63 +15:52:24.7
05:53:45.05 +15:09:38.0
05:53:06.34 +14:57:36.0
05:51:06.34 +15:03:05.9
05:51:24.40 +15:08:08.5
05:54:14.08 +15:13:42.7
06:04:04.16 +17:40:32.2
06:20:00.56 +17:12:18.2
05:57:32.63 +14:41:17.1
05:54:08.57 +14:53:55.7
05:57:11.85 +14:38:51.9
06:02:12.90 +14:59:52.0
06:06:52.06 +15:48:39.0
05:56:30.91 +12:09:19.9
06:03:42.69 +13:07:00.2
05:58:23.77 +11:50:43.6
###################################################################################
06:35:44.94 +11:17:01.3 -- asteroid (will NOT add it to exclusion list)
06:17:32.29 +16:47:23.0 -- not an asteroid (will add it to exclusion list)
06:02:38.33 +14:07:59.3 -- not an asteroid (will add it to exclusion list)
06:16:41.50 +14:25:10.4 -- not an asteroid (will add it to exclusion list)
06:15:49.41 +13:13:07.8 -- not an asteroid (will add it to exclusion list)
06:19:01.55 +14:21:47.0 -- not an asteroid (will add it to exclusion list)
05:54:48.72 +13:47:50.8 -- not an asteroid (will add it to exclusion list)
06:25:19.99 +15:08:17.2 -- not an asteroid (will add it to exclusion list)
06:16:49.33 +14:56:25.0 -- not an asteroid (will add it to exclusion list)
06:12:29.71 +12:51:00.4 -- not an asteroid (will add it to exclusion list)
06:08:08.32 +14:27:06.1 -- not an asteroid (will add it to exclusion list)
06:20:10.22 +12:07:10.0 -- not an asteroid (will add it to exclusion list)
06:04:08.81 +11:12:57.6 -- not an asteroid (will add it to exclusion list)
06:03:03.62 +13:25:03.3 -- not an asteroid (will add it to exclusion list)
06:07:50.05 +12:50:04.1 -- not an asteroid (will add it to exclusion list)
05:57:25.12 +15:34:07.5 -- not an asteroid (will add it to exclusion list)
05:58:51.50 +15:39:36.4 -- not an asteroid (will add it to exclusion list)
06:28:32.96 +15:25:10.6 -- not an asteroid (will add it to exclusion list)
05:50:29.23 +15:16:05.2 -- not an asteroid (will add it to exclusion list)
05:51:58.05 +15:48:26.5 -- not an asteroid (will add it to exclusion list)
05:55:21.81 +15:39:09.6 -- not an asteroid (will add it to exclusion list)
06:36:29.76 +16:46:34.6 -- not an asteroid (will add it to exclusion list)
06:21:43.51 +12:44:21.3 -- not an asteroid (will add it to exclusion list)
06:08:07.79 +15:55:02.4 -- not an asteroid (will add it to exclusion list)
06:07:08.77 +12:32:29.9 -- not an asteroid (will add it to exclusion list)
05:51:07.57 +10:13:07.3 -- not an asteroid (will add it to exclusion list)
06:20:58.24 +16:02:33.0 -- not an asteroid (will add it to exclusion list)
05:56:05.78 +17:53:51.3 -- not an asteroid (will add it to exclusion list)
05:57:50.52 +15:53:33.9 -- not an asteroid (will add it to exclusion list)
06:35:48.68 +18:02:11.9 -- not an asteroid (will add it to exclusion list)
06:35:19.20 +14:30:00.3 -- not an asteroid (will add it to exclusion list)
06:07:05.41 +10:57:47.1 -- not an asteroid (will add it to exclusion list)
05:52:23.96 +13:19:35.4 -- not an asteroid (will add it to exclusion list)
06:13:51.21 +16:29:05.2 -- not an asteroid (will add it to exclusion list)
06:00:30.08 +09:53:10.7 -- not an asteroid (will add it to exclusion list)
06:18:53.63 +17:20:32.0 -- not an asteroid (will add it to exclusion list)
06:41:08.40 +16:06:36.5 -- not an asteroid (will add it to exclusion list)
05:53:16.81 +14:42:25.5 -- not an asteroid (will add it to exclusion list)
06:10:22.30 +16:14:32.0 -- not an asteroid (will add it to exclusion list)
06:21:24.15 +14:10:53.8 -- not an asteroid (will add it to exclusion list)
05:57:35.34 +17:58:56.2 -- not an asteroid (will add it to exclusion list)
06:20:25.32 +17:59:14.9 -- not an asteroid (will add it to exclusion list)
06:40:42.95 +17:09:24.7 -- not an asteroid (will add it to exclusion list)
06:03:24.40 +14:38:53.8 -- not an asteroid (will add it to exclusion list)
06:20:41.97 +17:05:20.2 -- not an asteroid (will add it to exclusion list)
06:11:44.47 +17:21:10.7 -- not an asteroid (will add it to exclusion list)
05:57:38.21 +16:48:12.8 -- not an asteroid (will add it to exclusion list)
05:55:49.49 +17:04:43.7 -- not an asteroid (will add it to exclusion list)
06:26:09.52 +14:11:10.7 -- not an asteroid (will add it to exclusion list)
06:00:38.06 +15:37:20.1 -- not an asteroid (will add it to exclusion list)
06:20:06.66 +15:51:59.5 -- not an asteroid (will add it to exclusion list)
06:15:50.93 +17:58:53.9 -- not an asteroid (will add it to exclusion list)
06:21:19.04 +12:51:49.2 -- not an asteroid (will add it to exclusion list)
06:28:49.44 +15:22:57.9 -- not an asteroid (will add it to exclusion list)
06:25:36.63 +13:37:49.9 -- not an asteroid (will add it to exclusion list)
06:01:20.73 +13:05:22.2 -- not an asteroid (will add it to exclusion list)
06:13:39.34 +15:30:56.7 -- not an asteroid (will add it to exclusion list)
06:06:13.05 +16:19:25.1 -- not an asteroid (will add it to exclusion list)
05:57:00.14 +13:28:56.4 -- not an asteroid (will add it to exclusion list)
06:02:12.33 +12:06:05.4 -- not an asteroid (will add it to exclusion list)
05:55:30.14 +15:07:44.4 -- not an asteroid (will add it to exclusion list)
06:15:20.07 +14:59:21.8 -- not an asteroid (will add it to exclusion list)
05:53:57.36 +12:16:41.1 -- not an asteroid (will add it to exclusion list)
05:50:05.30 +10:34:52.5 -- not an asteroid (will add it to exclusion list)
06:02:09.71 +12:11:04.8 -- not an asteroid (will add it to exclusion list)
06:27:07.95 +16:55:01.9 -- not an asteroid (will add it to exclusion list)
05:58:18.72 +18:08:55.4 -- not an asteroid (will add it to exclusion list)
05:53:22.72 +12:06:18.0 -- not an asteroid (will add it to exclusion list)
05:57:16.62 +12:53:47.2 -- not an asteroid (will add it to exclusion list)
06:20:46.12 +17:46:19.4 -- not an asteroid (will add it to exclusion list)
06:10:32.47 +16:29:30.3 -- not an asteroid (will add it to exclusion list)
05:59:16.87 +12:05:09.6 -- not an asteroid (will add it to exclusion list)
05:51:37.51 +13:14:02.5 -- not an asteroid (will add it to exclusion list)
06:12:20.10 +10:02:03.9 -- not an asteroid (will add it to exclusion list)
05:53:57.38 +15:58:38.5 -- not an asteroid (will add it to exclusion list)
06:10:55.23 +18:14:13.8 -- not an asteroid (will add it to exclusion list)
05:58:27.39 +16:42:25.2 -- not an asteroid (will add it to exclusion list)
05:54:00.73 +14:50:42.4 -- not an asteroid (will add it to exclusion list)
06:34:16.98 +17:15:29.9 -- not an asteroid (will add it to exclusion list)
06:13:58.17 +14:27:25.2 -- not an asteroid (will add it to exclusion list)
06:13:27.44 +14:13:52.4 -- not an asteroid (will add it to exclusion list)
06:13:55.42 +12:05:34.8 -- not an asteroid (will add it to exclusion list)
06:29:40.32 +17:17:01.6 -- not an asteroid (will add it to exclusion list)
05:52:18.18 +15:51:58.7 -- not an asteroid (will add it to exclusion list)
06:02:24.65 +14:17:47.4 -- not an asteroid (will add it to exclusion list)
06:24:13.84 +15:54:30.3 -- not an asteroid (will add it to exclusion list)
06:18:02.62 +17:41:17.8 -- not an asteroid (will add it to exclusion list)
06:38:34.20 +17:37:22.6 -- not an asteroid (will add it to exclusion list)
05:54:41.60 +12:22:48.9 -- not an asteroid (will add it to exclusion list)
06:11:23.67 +14:49:43.7 -- 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)
06:13:49.73 +12:47:06.0 -- not an asteroid (will add it to exclusion list)
05:55:31.07 +15:11:03.3 -- not an asteroid (will add it to exclusion list)
06:09:12.84 +15:40:25.5 -- not an asteroid (will add it to exclusion list)
05:51:38.55 +14:47:55.2 -- not an asteroid (will add it to exclusion list)
06:13:23.68 +17:13:26.6 -- not an asteroid (will add it to exclusion list)
05:51:05.88 +15:39:53.7 -- not an asteroid (will add it to exclusion list)
06:00:53.36 +14:53:46.9 -- not an asteroid (will add it to exclusion list)
05:55:47.09 +14:33:50.9 -- not an asteroid (will add it to exclusion list)
06:00:25.20 +16:41:37.4 -- not an asteroid (will add it to exclusion list)
06:27:09.44 +15:25:23.6 -- not an asteroid (will add it to exclusion list)
06:38:45.68 +13:41:32.4 -- not an asteroid (will add it to exclusion list)
06:32:06.11 +18:09:37.2 -- not an asteroid (will add it to exclusion list)
06:13:48.73 +12:57:35.1 -- not an asteroid (will add it to exclusion list)
05:57:25.91 +11:32:51.5 -- not an asteroid (will add it to exclusion list)
06:14:38.16 +13:49:46.1 -- not an asteroid (will add it to exclusion list)
06:39:55.14 +13:35:03.6 -- not an asteroid (will add it to exclusion list)
06:01:02.76 +13:48:59.6 -- not an asteroid (will add it to exclusion list)
06:35:42.69 +11:30:05.7 -- not an asteroid (will add it to exclusion list)
06:41:18.50 +18:02:07.2 -- not an asteroid (will add it to exclusion list)
05:49:55.21 +12:51:44.4 -- not an asteroid (will add it to exclusion list)
06:31:42.82 +11:11:14.9 -- not an asteroid (will add it to exclusion list)
06:36:11.37 +17:16:23.4 -- not an asteroid (will add it to exclusion list)
05:55:57.28 +16:32:15.5 -- not an asteroid (will add it to exclusion list)
06:25:55.13 +15:51:16.3 -- not an asteroid (will add it to exclusion list)
06:40:48.75 +17:56:48.8 -- not an asteroid (will add it to exclusion list)
06:26:36.81 +17:47:21.7 -- not an asteroid (will add it to exclusion list)
05:49:25.37 +10:51:15.1 -- not an asteroid (will add it to exclusion list)
05:50:34.10 +14:49:09.8 -- asteroid (will NOT add it to exclusion list)
06:41:51.58 +15:27:19.7 -- not an asteroid (will add it to exclusion list)
06:06:26.73 +10:44:52.7 -- not an asteroid (will add it to exclusion list)
05:56:53.26 +14:50:24.2 -- asteroid (will NOT add it to exclusion list)
06:16:27.36 +16:42:37.2 -- not an asteroid (will add it to exclusion list)
06:03:45.61 +14:20:46.4 -- not an asteroid (will add it to exclusion list)
06:30:33.66 +17:55:15.4 -- asteroid (will NOT add it to exclusion list)
06:16:45.41 +15:33:25.8 -- not an asteroid (will add it to exclusion list)
06:10:12.01 +17:42:33.7 -- not an asteroid (will add it to exclusion list)
06:23:25.04 +17:30:59.4 -- not an asteroid (will add it to exclusion list)
06:19:42.39 +15:59:26.3 -- not an asteroid (will add it to exclusion list)
06:11:37.59 +13:51:44.9 -- not an asteroid (will add it to exclusion list)
06:08:41.20 +17:23:37.2 -- not an asteroid (will add it to exclusion list)
06:13:09.91 +18:03:25.5 -- not an asteroid (will add it to exclusion list)
06:05:30.91 +16:17:58.0 -- not an asteroid (will add it to exclusion list)
05:57:13.90 +17:30:31.9 -- not an asteroid (will add it to exclusion list)
06:10:33.18 +17:47:20.1 -- not an asteroid (will add it to exclusion list)
05:57:47.60 +14:19:57.4 -- asteroid (will NOT add it to exclusion list)
06:17:11.15 +15:50:14.3 -- not an asteroid (will add it to exclusion list)
05:56:44.14 +17:00:11.1 -- not an asteroid (will add it to exclusion list)
06:18:18.15 +14:22:19.4 -- not an asteroid (will add it to exclusion list)
06:16:56.03 +15:17:01.8 -- not an asteroid (will add it to exclusion list)
06:10:55.69 +15:29:38.5 -- not an asteroid (will add it to exclusion list)
06:09:52.24 +11:19:55.0 -- not an asteroid (will add it to exclusion list)
06:35:06.77 +12:37:58.3 -- not an asteroid (will add it to exclusion list)
06:37:54.50 +17:30:25.6 -- not an asteroid (will add it to exclusion list)
06:20:46.44 +15:18:14.8 -- not an asteroid (will add it to exclusion list)
06:22:11.62 +16:05:21.3 -- not an asteroid (will add it to exclusion list)
05:56:26.65 +17:40:49.6 -- not an asteroid (will add it to exclusion list)
06:25:09.44 +15:58:53.2 -- not an asteroid (will add it to exclusion list)
06:07:01.07 +10:58:45.5 -- not an asteroid (will add it to exclusion list)
06:10:14.13 +13:48:21.8 -- not an asteroid (will add it to exclusion list)
06:02:06.73 +15:11:09.4 -- not an asteroid (will add it to exclusion list)
06:12:57.12 +17:26:20.6 -- not an asteroid (will add it to exclusion list)
06:17:52.61 +15:42:08.3 -- not an asteroid (will add it to exclusion list)
05:57:12.71 +17:39:14.8 -- not an asteroid (will add it to exclusion list)
06:27:55.34 +17:41:36.1 -- not an asteroid (will add it to exclusion list)
06:06:27.04 +10:44:01.4 -- not an asteroid (will add it to exclusion list)
06:10:30.91 +14:52:41.1 -- not an asteroid (will add it to exclusion list)
06:12:28.10 +15:20:03.5 -- not an asteroid (will add it to exclusion list)
06:29:40.10 +11:43:01.9 -- not an asteroid (will add it to exclusion list)
06:07:20.22 +16:45:35.4 -- not an asteroid (will add it to exclusion list)
06:14:37.25 +16:02:29.7 -- not an asteroid (will add it to exclusion list)
06:38:54.79 +15:11:20.6 -- not an asteroid (will add it to exclusion list)
05:54:13.85 +13:11:37.5 -- not an asteroid (will add it to exclusion list)
06:35:02.86 +17:42:00.9 -- not an asteroid (will add it to exclusion list)
05:56:33.25 +15:11:30.2 -- not an asteroid (will add it to exclusion list)
06:22:05.27 +17:47:57.3 -- not an asteroid (will add it to exclusion list)
06:27:44.25 +17:39:43.5 -- not an asteroid (will add it to exclusion list)
06:19:14.38 +17:25:24.8 -- not an asteroid (will add it to exclusion list)
06:16:19.85 +14:31:16.3 -- not an asteroid (will add it to exclusion list)
05:54:35.46 +12:10:02.2 -- not an asteroid (will add it to exclusion list)
06:00:20.47 +15:32:27.5 -- not an asteroid (will add it to exclusion list)
05:59:54.86 +17:17:28.4 -- not an asteroid (will add it to exclusion list)
06:14:42.27 +15:10:59.5 -- not an asteroid (will add it to exclusion list)
05:58:48.35 +13:38:11.6 -- not an asteroid (will add it to exclusion list)
05:57:00.05 +17:55:40.0 -- not an asteroid (will add it to exclusion list)
06:34:47.09 +15:31:01.1 -- not an asteroid (will add it to exclusion list)
06:15:28.00 +14:23:53.4 -- not an asteroid (will add it to exclusion list)
05:54:30.48 +12:57:30.9 -- not an asteroid (will add it to exclusion list)
06:20:57.18 +16:50:14.0 -- not an asteroid (will add it to exclusion list)
06:31:32.15 +18:03:36.5 -- not an asteroid (will add it to exclusion list)
06:11:37.15 +15:28:26.2 -- not an asteroid (will add it to exclusion list)
05:54:22.03 +15:30:54.7 -- not an asteroid (will add it to exclusion list)
05:49:14.20 +14:41:49.7 -- not an asteroid (will add it to exclusion list)
05:58:26.34 +15:59:27.6 -- not an asteroid (will add it to exclusion list)
06:19:47.07 +16:38:51.9 -- not an asteroid (will add it to exclusion list)
05:57:13.12 +12:48:33.4 -- not an asteroid (will add it to exclusion list)
06:06:58.48 +14:36:07.9 -- not an asteroid (will add it to exclusion list)
06:12:31.18 +15:20:12.7 -- not an asteroid (will add it to exclusion list)
06:03:52.36 +14:59:05.9 -- not an asteroid (will add it to exclusion list)
06:18:54.41 +11:33:57.4 -- not an asteroid (will add it to exclusion list)
06:21:38.01 +12:02:48.8 -- not an asteroid (will add it to exclusion list)
05:49:28.23 +11:30:41.3 -- not an asteroid (will add it to exclusion list)
06:12:26.70 +15:00:24.4 -- not an asteroid (will add it to exclusion list)
06:02:32.64 +14:05:00.5 -- not an asteroid (will add it to exclusion list)
06:04:53.18 +10:54:04.3 -- not an asteroid (will add it to exclusion list)
05:57:33.73 +15:38:38.1 -- not an asteroid (will add it to exclusion list)
06:10:46.67 +14:47:19.1 -- not an asteroid (will add it to exclusion list)
05:48:53.22 +10:13:09.7 -- not an asteroid (will add it to exclusion list)
05:56:30.04 +12:01:33.2 -- not an asteroid (will add it to exclusion list)
06:07:36.39 +10:59:23.3 -- not an asteroid (will add it to exclusion list)
05:50:55.72 +13:52:50.5 -- not an asteroid (will add it to exclusion list)
06:19:12.12 +12:45:05.8 -- not an asteroid (will add it to exclusion list)
06:41:44.73 +15:13:17.5 -- not an asteroid (will add it to exclusion list)
06:23:49.23 +16:28:13.4 -- not an asteroid (will add it to exclusion list)
06:11:05.87 +16:19:10.2 -- not an asteroid (will add it to exclusion list)
05:50:50.16 +14:25:32.6 -- not an asteroid (will add it to exclusion list)
06:01:37.66 +14:43:11.3 -- not an asteroid (will add it to exclusion list)
05:55:56.95 +15:40:28.5 -- not an asteroid (will add it to exclusion list)
05:56:21.65 +17:58:16.6 -- not an asteroid (will add it to exclusion list)
06:20:58.57 +14:41:22.8 -- not an asteroid (will add it to exclusion list)
05:58:16.45 +16:05:42.7 -- not an asteroid (will add it to exclusion list)
05:48:53.57 +10:23:25.0 -- not an asteroid (will add it to exclusion list)
05:58:03.65 +15:30:43.4 -- not an asteroid (will add it to exclusion list)
06:26:05.78 +16:32:36.8 -- not an asteroid (will add it to exclusion list)
06:18:06.36 +11:26:20.6 -- not an asteroid (will add it to exclusion list)
06:25:59.18 +14:56:44.5 -- not an asteroid (will add it to exclusion list)
06:12:49.42 +11:40:07.8 -- not an asteroid (will add it to exclusion list)
06:09:15.54 +11:12:53.5 -- not an asteroid (will add it to exclusion list)
06:05:26.55 +12:45:45.3 -- not an asteroid (will add it to exclusion list)
06:00:57.42 +16:27:52.8 -- not an asteroid (will add it to exclusion list)
05:57:34.57 +11:12:21.5 -- not an asteroid (will add it to exclusion list)
06:11:09.02 +17:31:04.6 -- not an asteroid (will add it to exclusion list)
06:13:14.11 +13:29:52.0 -- not an asteroid (will add it to exclusion list)
05:50:37.80 +12:00:50.3 -- not an asteroid (will add it to exclusion list)
06:28:04.93 +14:04:45.4 -- not an asteroid (will add it to exclusion list)
05:51:00.49 +13:29:08.0 -- not an asteroid (will add it to exclusion list)
06:19:04.28 +16:47:19.9 -- not an asteroid (will add it to exclusion list)
06:05:37.30 +17:10:43.6 -- not an asteroid (will add it to exclusion list)
05:53:09.28 +11:49:52.4 -- not an asteroid (will add it to exclusion list)
06:14:02.40 +15:01:15.6 -- not an asteroid (will add it to exclusion list)
06:29:32.69 +17:39:52.8 -- not an asteroid (will add it to exclusion list)
05:50:32.94 +15:45:58.9 -- not an asteroid (will add it to exclusion list)
06:12:18.19 +15:12:21.7 -- not an asteroid (will add it to exclusion list)
06:13:16.49 +15:43:24.4 -- not an asteroid (will add it to exclusion list)
06:25:40.26 +17:47:38.4 -- not an asteroid (will add it to exclusion list)
06:09:55.66 +14:26:06.5 -- not an asteroid (will add it to exclusion list)
06:01:34.55 +16:08:07.9 -- not an asteroid (will add it to exclusion list)
06:02:46.01 +11:05:17.8 -- not an asteroid (will add it to exclusion list)
05:59:14.13 +16:16:41.1 -- not an asteroid (will add it to exclusion list)
06:19:02.10 +16:47:08.2 -- not an asteroid (will add it to exclusion list)
05:51:57.97 +14:40:17.5 -- not an asteroid (will add it to exclusion list)
05:50:16.03 +13:54:05.4 -- not an asteroid (will add it to exclusion list)
05:53:56.26 +15:51:26.8 -- not an asteroid (will add it to exclusion list)
06:27:51.81 +16:41:07.0 -- not an asteroid (will add it to exclusion list)
05:53:13.27 +14:40:26.4 -- not an asteroid (will add it to exclusion list)
05:51:52.97 +15:55:28.7 -- not an asteroid (will add it to exclusion list)
06:16:58.71 +18:09:12.0 -- not an asteroid (will add it to exclusion list)
06:17:35.48 +14:21:38.5 -- not an asteroid (will add it to exclusion list)
06:26:03.55 +16:32:25.5 -- not an asteroid (will add it to exclusion list)
06:01:33.58 +16:49:51.0 -- not an asteroid (will add it to exclusion list)
06:18:42.38 +17:53:59.0 -- not an asteroid (will add it to exclusion list)
06:20:51.87 +17:05:08.9 -- not an asteroid (will add it to exclusion list)
05:52:58.21 +15:17:40.7 -- not an asteroid (will add it to exclusion list)
06:06:48.58 +16:40:37.3 -- not an asteroid (will add it to exclusion list)
06:11:58.99 +17:22:43.8 -- not an asteroid (will add it to exclusion list)
05:56:29.76 +15:23:10.1 -- not an asteroid (will add it to exclusion list)
06:14:08.37 +17:22:59.0 -- not an asteroid (will add it to exclusion list)
05:56:56.29 +16:55:37.5 -- not an asteroid (will add it to exclusion list)
05:59:56.14 +11:30:33.4 -- not an asteroid (will add it to exclusion list)
06:01:42.15 +16:14:30.0 -- not an asteroid (will add it to exclusion list)
05:55:47.25 +14:48:04.2 -- not an asteroid (will add it to exclusion list)
06:14:35.32 +13:49:52.5 -- not an asteroid (will add it to exclusion list)
06:18:28.87 +14:20:26.5 -- not an asteroid (will add it to exclusion list)
06:06:22.14 +14:21:40.1 -- not an asteroid (will add it to exclusion list)
06:00:22.07 +10:05:27.1 -- asteroid (will NOT add it to exclusion list)
06:18:52.50 +13:48:26.1 -- not an asteroid (will add it to exclusion list)
06:05:27.21 +10:56:04.5 -- not an asteroid (will add it to exclusion list)
06:11:38.95 +16:33:10.4 -- not an asteroid (will add it to exclusion list)
06:39:09.96 +13:11:14.6 -- not an asteroid (will add it to exclusion list)
06:01:17.73 +15:06:07.6 -- not an asteroid (will add it to exclusion list)
06:16:11.26 +14:06:20.4 -- not an asteroid (will add it to exclusion list)
06:08:55.85 +17:07:40.2 -- not an asteroid (will add it to exclusion list)
06:01:32.33 +14:49:01.0 -- not an asteroid (will add it to exclusion list)
06:15:38.04 +17:53:12.8 -- not an asteroid (will add it to exclusion list)
05:58:07.88 +17:09:02.1 -- not an asteroid (will add it to exclusion list)
06:10:40.74 +15:14:02.4 -- not an asteroid (will add it to exclusion list)
06:25:33.70 +17:35:15.0 -- not an asteroid (will add it to exclusion list)
06:01:19.57 +15:34:36.3 -- not an asteroid (will add it to exclusion list)
06:12:51.31 +13:17:02.7 -- not an asteroid (will add it to exclusion list)
06:39:17.07 +15:47:13.6 -- not an asteroid (will add it to exclusion list)
05:52:24.03 +13:07:42.6 -- not an asteroid (will add it to exclusion list)
06:36:16.00 +17:59:28.7 -- not an asteroid (will add it to exclusion list)
06:20:14.51 +13:20:23.6 -- not an asteroid (will add it to exclusion list)
06:13:50.87 +14:44:31.4 -- not an asteroid (will add it to exclusion list)
06:16:27.29 +14:57:43.4 -- not an asteroid (will add it to exclusion list)
05:49:53.48 +12:29:46.2 -- not an asteroid (will add it to exclusion list)
06:06:01.07 +16:53:34.0 -- not an asteroid (will add it to exclusion list)
06:14:07.62 +18:00:35.3 -- not an asteroid (will add it to exclusion list)
06:15:51.77 +13:13:57.6 -- not an asteroid (will add it to exclusion list)
06:04:27.92 +16:29:13.6 -- not an asteroid (will add it to exclusion list)
05:52:31.28 +12:19:33.1 -- not an asteroid (will add it to exclusion list)
05:55:56.68 +14:38:13.5 -- not an asteroid (will add it to exclusion list)
06:10:29.67 +16:02:29.5 -- not an asteroid (will add it to exclusion list)
05:50:03.82 +10:24:32.0 -- not an asteroid (will add it to exclusion list)
06:17:27.92 +11:05:42.8 -- asteroid (will NOT add it to exclusion list)
06:10:25.17 +16:38:52.0 -- not an asteroid (will add it to exclusion list)
06:20:25.62 +16:52:34.9 -- not an asteroid (will add it to exclusion list)
05:58:52.31 +13:37:23.5 -- not an asteroid (will add it to exclusion list)
06:25:04.28 +16:36:40.6 -- not an asteroid (will add it to exclusion list)
05:49:46.29 +14:47:43.5 -- not an asteroid (will add it to exclusion list)
06:07:09.47 +16:42:47.4 -- not an asteroid (will add it to exclusion list)
05:58:56.45 +18:06:46.5 -- not an asteroid (will add it to exclusion list)
05:59:52.66 +12:19:21.9 -- not an asteroid (will add it to exclusion list)
06:06:04.83 +13:40:16.8 -- not an asteroid (will add it to exclusion list)
06:11:18.41 +14:47:53.9 -- not an asteroid (will add it to exclusion list)
05:56:54.46 +15:03:06.2 -- not an asteroid (will add it to exclusion list)
06:27:52.40 +16:41:35.9 -- not an asteroid (will add it to exclusion list)
06:25:51.85 +15:01:10.9 -- not an asteroid (will add it to exclusion list)
05:58:27.90 +15:59:40.8 -- not an asteroid (will add it to exclusion list)
05:48:20.40 +13:06:39.3 -- not an asteroid (will add it to exclusion list)
06:10:34.15 +18:09:01.8 -- not an asteroid (will add it to exclusion list)
06:38:54.23 +17:47:26.8 -- not an asteroid (will add it to exclusion list)
06:27:31.24 +15:16:12.7 -- not an asteroid (will add it to exclusion list)
05:52:03.71 +15:17:56.9 -- not an asteroid (will add it to exclusion list)
05:49:09.18 +15:28:21.4 -- not an asteroid (will add it to exclusion list)
06:11:39.60 +16:27:38.5 -- not an asteroid (will add it to exclusion list)
05:58:55.65 +14:23:33.8 -- not an asteroid (will add it to exclusion list)
06:19:36.65 +17:40:28.7 -- not an asteroid (will add it to exclusion list)
06:10:28.05 +13:50:01.6 -- not an asteroid (will add it to exclusion list)
05:55:50.17 +17:41:15.7 -- not an asteroid (will add it to exclusion list)
05:49:45.62 +14:44:54.6 -- not an asteroid (will add it to exclusion list)
05:57:35.77 +15:03:49.6 -- not an asteroid (will add it to exclusion list)
05:59:50.35 +16:54:20.2 -- not an asteroid (will add it to exclusion list)
05:58:04.82 +13:32:09.6 -- not an asteroid (will add it to exclusion list)
05:57:41.34 +17:40:40.5 -- not an asteroid (will add it to exclusion list)
06:01:56.65 +16:44:38.7 -- not an asteroid (will add it to exclusion list)
05:50:36.42 +14:31:42.7 -- not an asteroid (will add it to exclusion list)
06:00:53.07 +12:13:41.6 -- not an asteroid (will add it to exclusion list)
06:06:05.08 +13:21:02.4 -- not an asteroid (will add it to exclusion list)
06:00:38.99 +15:55:36.4 -- not an asteroid (will add it to exclusion list)
05:56:38.86 +17:44:21.4 -- not an asteroid (will add it to exclusion list)
06:19:59.31 +17:10:05.9 -- not an asteroid (will add it to exclusion list)
05:54:24.85 +15:55:48.1 -- not an asteroid (will add it to exclusion list)
05:56:30.45 +15:24:06.3 -- not an asteroid (will add it to exclusion list)
05:58:28.09 +17:33:01.5 -- not an asteroid (will add it to exclusion list)
05:53:45.27 +15:46:35.8 -- not an asteroid (will add it to exclusion list)
06:00:54.64 +15:22:19.2 -- not an asteroid (will add it to exclusion list)
06:15:24.32 +13:24:20.3 -- not an asteroid (will add it to exclusion list)
05:59:39.43 +13:09:23.1 -- not an asteroid (will add it to exclusion list)
06:01:32.19 +16:40:16.4 -- not an asteroid (will add it to exclusion list)
06:10:33.47 +16:28:35.0 -- not an asteroid (will add it to exclusion list)
05:48:48.99 +15:03:36.3 -- not an asteroid (will add it to exclusion list)
05:56:31.53 +16:33:11.6 -- not an asteroid (will add it to exclusion list)
06:02:07.05 +16:19:41.2 -- not an asteroid (will add it to exclusion list)
06:08:01.86 +15:33:58.0 -- not an asteroid (will add it to exclusion list)
05:50:06.04 +12:53:14.1 -- not an asteroid (will add it to exclusion list)
05:52:28.71 +14:24:30.1 -- not an asteroid (will add it to exclusion list)
06:01:17.11 +15:30:04.1 -- not an asteroid (will add it to exclusion list)
05:55:42.04 +14:41:21.9 -- not an asteroid (will add it to exclusion list)
05:58:42.60 +11:51:00.9 -- asteroid (will NOT add it to exclusion list)
05:58:09.45 +17:20:40.6 -- not an asteroid (will add it to exclusion list)
06:02:05.99 +16:03:13.3 -- not an asteroid (will add it to exclusion list)
06:10:07.81 +15:00:28.2 -- not an asteroid (will add it to exclusion list)
05:52:47.63 +15:52:24.7 -- not an asteroid (will add it to exclusion list)
05:53:45.05 +15:09:38.0 -- not an asteroid (will add it to exclusion list)
05:53:06.34 +14:57:36.0 -- not an asteroid (will add it to exclusion list)
05:51:06.34 +15:03:05.9 -- not an asteroid (will add it to exclusion list)
05:51:24.40 +15:08:08.5 -- not an asteroid (will add it to exclusion list)
05:54:14.08 +15:13:42.7 -- not an asteroid (will add it to exclusion list)
06:04:04.16 +17:40:32.2 -- not an asteroid (will add it to exclusion list)
06:20:00.56 +17:12:18.2 -- not an asteroid (will add it to exclusion list)
05:57:32.63 +14:41:17.1 -- not an asteroid (will add it to exclusion list)
05:54:08.57 +14:53:55.7 -- not an asteroid (will add it to exclusion list)
05:57:11.85 +14:38:51.9 -- not an asteroid (will add it to exclusion list)
06:02:12.90 +14:59:52.0 -- not an asteroid (will add it to exclusion list)
06:06:52.06 +15:48:39.0 -- not an asteroid (will add it to exclusion list)
05:56:30.91 +12:09:19.9 -- not an asteroid (will add it to exclusion list)
06:03:42.69 +13:07:00.2 -- not an asteroid (will add it to exclusion list)
05:58:23.77 +11:50:43.6 -- asteroid (will NOT add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:48:20.40 +13:06:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:48.99 +15:03:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.22 +10:13:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.57 +10:23:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:09.18 +15:28:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:14.20 +14:41:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:25.37 +10:51:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:28.23 +11:30:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:45.62 +14:44:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:46.29 +14:47:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:53.48 +12:29:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:55.21 +12:51:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:03.82 +10:24:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:05.30 +10:34:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:06.04 +12:53:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:16.03 +13:54:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:29.23 +15:16:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:32.94 +15:45:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:36.42 +14:31:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:37.80 +12:00:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:50.16 +14:25:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:55.72 +13:52:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:00.49 +13:29:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:05.88 +15:39:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:06.34 +15:03:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:07.57 +10:13:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:24.40 +15:08:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:37.51 +13:14:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:38.55 +14:47:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:52.97 +15:55:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:57.97 +14:40:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:58.05 +15:48:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:03.71 +15:17:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:18.18 +15:51:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:23.96 +13:19:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:24.03 +13:07:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:28.71 +14:24:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:31.28 +12:19:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:47.63 +15:52:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:58.21 +15:17:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:06.34 +14:57:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:09.28 +11:49:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:13.27 +14:40:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:16.81 +14:42:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:22.72 +12:06:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:45.05 +15:09:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:45.27 +15:46:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:56.26 +15:51:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:57.36 +12:16:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:57.38 +15:58:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:00.73 +14:50:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:08.57 +14:53:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:13.85 +13:11:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:14.08 +15:13:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:22.03 +15:30:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:24.85 +15:55:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:30.48 +12:57:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:35.46 +12:10:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:41.60 +12:22:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:48.72 +13:47:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:21.81 +15:39:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:30.14 +15:07:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:31.07 +15:11:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:42.04 +14:41:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:47.09 +14:33:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:47.25 +14:48:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:49.49 +17:04:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:50.17 +17:41:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:56.68 +14:38:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:56.95 +15:40:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:57.28 +16:32:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:05.78 +17:53:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:21.65 +17:58:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:26.65 +17:40:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:29.76 +15:23:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:30.04 +12:01:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:30.45 +15:24:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:30.91 +12:09:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:31.53 +16:33:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:33.25 +15:11:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:38.86 +17:44:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:44.14 +17:00:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:54.46 +15:03:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:56.29 +16:55:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:00.05 +17:55:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:00.14 +13:28:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:11.85 +14:38:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.71 +17:39:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:13.12 +12:48:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:13.90 +17:30:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:16.62 +12:53:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:25.12 +15:34:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:25.91 +11:32:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:32.63 +14:41:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:33.73 +15:38:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:34.57 +11:12:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:35.34 +17:58:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:35.77 +15:03:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:38.21 +16:48:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:41.34 +17:40:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:50.52 +15:53:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:03.65 +15:30:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:04.82 +13:32:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:07.88 +17:09:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.45 +17:20:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:16.45 +16:05:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:18.72 +18:08:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:26.34 +15:59:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:27.39 +16:42:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:27.90 +15:59:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:28.09 +17:33:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:48.35 +13:38:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:51.50 +15:39:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:52.31 +13:37:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:55.65 +14:23:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:56.45 +18:06:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:14.13 +16:16:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:16.87 +12:05:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:39.43 +13:09:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:50.35 +16:54:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:52.66 +12:19:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:54.86 +17:17:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:56.14 +11:30:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:20.47 +15:32:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:25.20 +16:41:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:30.08 +09:53:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:38.06 +15:37:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:38.99 +15:55:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:53.07 +12:13:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:53.36 +14:53:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:54.64 +15:22:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:57.42 +16:27:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:02.76 +13:48:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:17.11 +15:30:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:17.73 +15:06:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:19.57 +15:34:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:20.73 +13:05:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:32.19 +16:40:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:32.33 +14:49:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:33.58 +16:49:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:34.55 +16:08:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:37.66 +14:43:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:42.15 +16:14:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:56.65 +16:44:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:05.99 +16:03:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:06.73 +15:11:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:07.05 +16:19:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:09.71 +12:11:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:12.33 +12:06:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:12.90 +14:59:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:24.65 +14:17:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.64 +14:05:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:38.33 +14:07:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:46.01 +11:05:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:03.62 +13:25:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:24.40 +14:38:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:42.69 +13:07:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:45.61 +14:20:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:52.36 +14:59:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:04.16 +17:40:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:08.81 +11:12:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:27.92 +16:29:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:53.18 +10:54:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:26.55 +12:45:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:27.21 +10:56:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:30.91 +16:17:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:37.30 +17:10:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:01.07 +16:53:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:04.83 +13:40:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:05.08 +13:21:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:13.05 +16:19:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:22.14 +14:21:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:26.73 +10:44:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:27.04 +10:44:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:48.58 +16:40:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:52.06 +15:48:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:58.48 +14:36:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:01.07 +10:58:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:05.41 +10:57:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:08.77 +12:32:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:09.47 +16:42:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:20.22 +16:45:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:36.39 +10:59:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:50.05 +12:50:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:01.86 +15:33:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:07.79 +15:55:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:08.32 +14:27:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:41.20 +17:23:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:55.85 +17:07:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:12.84 +15:40:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:15.54 +11:12:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:52.24 +11:19:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:55.66 +14:26:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:07.81 +15:00:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:12.01 +17:42:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:14.13 +13:48:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:22.30 +16:14:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:25.17 +16:38:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:28.05 +13:50:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:29.67 +16:02:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:30.91 +14:52:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:32.47 +16:29:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:33.18 +17:47:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:33.47 +16:28:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:34.15 +18:09:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:40.74 +15:14:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:46.67 +14:47:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:55.23 +18:14:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:55.69 +15:29:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:05.87 +16:19:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:09.02 +17:31:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:18.41 +14:47:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:23.67 +14:49:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:37.15 +15:28:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:37.59 +13:51:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:38.95 +16:33:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:39.60 +16:27:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:44.47 +17:21:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:58.99 +17:22:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:18.19 +15:12:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:20.10 +10:02:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:26.70 +15:00:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:28.10 +15:20:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:29.71 +12:51:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:31.18 +15:20:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:49.42 +11:40:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:51.31 +13:17:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:57.12 +17:26:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:09.91 +18:03:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:14.11 +13:29:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:16.49 +15:43:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:23.68 +17:13:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:27.44 +14:13:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:39.34 +15:30:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:48.73 +12:57:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:49.73 +12:47:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:50.87 +14:44:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:51.21 +16:29:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:55.42 +12:05:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:58.17 +14:27:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:02.40 +15:01:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:07.62 +18:00:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:08.37 +17:22:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:35.32 +13:49:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:37.25 +16:02:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:38.16 +13:49:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:42.27 +15:10:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:20.07 +14:59:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:24.32 +13:24:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:28.00 +14:23:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:38.04 +17:53:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:49.41 +13:13:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:50.93 +17:58:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:51.77 +13:13:57.6 -- 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)
06:16:11.26 +14:06:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:19.85 +14:31:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:27.29 +14:57:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:27.36 +16:42:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:41.50 +14:25:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:45.41 +15:33:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:49.33 +14:56:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:56.03 +15:17:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:58.71 +18:09:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:11.15 +15:50:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:32.29 +16:47:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:35.48 +14:21:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:52.61 +15:42:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:02.62 +17:41:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:06.36 +11:26:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:18.15 +14:22:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:28.87 +14:20:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:42.38 +17:53:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:52.50 +13:48:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:53.63 +17:20:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:54.41 +11:33:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:01.55 +14:21:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:02.10 +16:47:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:04.28 +16:47:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:12.12 +12:45:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:14.38 +17:25:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:36.65 +17:40:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:42.39 +15:59:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:47.07 +16:38:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:59.31 +17:10:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:00.56 +17:12:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:06.66 +15:51:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:10.22 +12:07:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:14.51 +13:20:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:25.32 +17:59:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:25.62 +16:52:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:41.97 +17:05:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:46.12 +17:46:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:46.44 +15:18:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:51.87 +17:05:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:57.18 +16:50:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:58.24 +16:02:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:58.57 +14:41:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:19.04 +12:51:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:24.15 +14:10:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:38.01 +12:02:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:43.51 +12:44:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:05.27 +17:47:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:11.62 +16:05:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:25.04 +17:30:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:49.23 +16:28:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:13.84 +15:54:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:04.28 +16:36:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:09.44 +15:58:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:19.99 +15:08:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:33.70 +17:35:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:36.63 +13:37:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:40.26 +17:47:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:51.85 +15:01:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:55.13 +15:51:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:59.18 +14:56:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:03.55 +16:32:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:05.78 +16:32:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:09.52 +14:11:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:36.81 +17:47:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:07.95 +16:55:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:09.44 +15:25:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:31.24 +15:16:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:44.25 +17:39:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:51.81 +16:41:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:52.40 +16:41:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:55.34 +17:41:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:04.93 +14:04:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:32.96 +15:25:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:49.44 +15:22:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:32.69 +17:39:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:40.10 +11:43:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:40.32 +17:17:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:32.15 +18:03:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:42.82 +11:11:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:06.11 +18:09:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:16.98 +17:15:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:47.09 +15:31:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:02.86 +17:42:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:06.77 +12:37:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:19.20 +14:30:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:42.69 +11:30:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:48.68 +18:02:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:11.37 +17:16:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:16.00 +17:59:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:29.76 +16:46:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:54.50 +17:30:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:34.20 +17:37:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:45.68 +13:41:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:54.23 +17:47:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:54.79 +15:11:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:09.96 +13:11:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:17.07 +15:47:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:55.14 +13:35:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:42.95 +17:09:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:48.75 +17:56:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:08.40 +16:06:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:18.50 +18:02:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:44.73 +15:13:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:51.58 +15:27:19.7 -- 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)
05:48:20.40 +13:06:39.3 -- not a known variable star
05:48:48.99 +15:03:36.3 -- not a known variable star
05:48:53.22 +10:13:09.7 -- not a known variable star
05:48:53.57 +10:23:25.0 -- not a known variable star
05:49:09.18 +15:28:21.4 -- not a known variable star
05:49:14.20 +14:41:49.7 -- a known variable star
05:49:25.37 +10:51:15.1 -- not a known variable star
05:49:28.23 +11:30:41.3 -- not a known variable star
05:49:45.62 +14:44:54.6 -- not a known variable star
05:49:46.29 +14:47:43.5 -- a known variable star
05:49:53.48 +12:29:46.2 -- not a known variable star
05:49:55.21 +12:51:44.4 -- not a known variable star
05:50:03.82 +10:24:32.0 -- a known variable star
05:50:05.30 +10:34:52.5 -- not a known variable star
05:50:06.04 +12:53:14.1 -- a known variable star
05:50:16.03 +13:54:05.4 -- not a known variable star
05:50:29.23 +15:16:05.2 -- not a known variable star
05:50:32.94 +15:45:58.9 -- not a known variable star
05:50:36.42 +14:31:42.7 -- not a known variable star
05:50:37.80 +12:00:50.3 -- not a known variable star
05:50:50.16 +14:25:32.6 -- not a known variable star
05:50:55.72 +13:52:50.5 -- not a known variable star
05:51:00.49 +13:29:08.0 -- a known variable star
05:51:05.88 +15:39:53.7 -- not a known variable star
05:51:06.34 +15:03:05.9 -- not a known variable star
05:51:07.57 +10:13:07.3 -- not a known variable star
05:51:24.40 +15:08:08.5 -- not a known variable star
05:51:37.51 +13:14:02.5 -- a known variable star
05:51:38.55 +14:47:55.2 -- a known variable star
05:51:52.97 +15:55:28.7 -- not a known variable star
05:51:57.97 +14:40:17.5 -- not a known variable star
05:51:58.05 +15:48:26.5 -- not a known variable star
05:52:03.71 +15:17:56.9 -- not a known variable star
05:52:18.18 +15:51:58.7 -- not a known variable star
05:52:23.96 +13:19:35.4 -- not a known variable star
05:52:24.03 +13:07:42.6 -- not a known variable star
05:52:28.71 +14:24:30.1 -- not a known variable star
05:52:31.28 +12:19:33.1 -- not a known variable star
05:52:47.63 +15:52:24.7 -- not a known variable star
05:52:58.21 +15:17:40.7 -- not a known variable star
05:53:06.34 +14:57:36.0 -- not a known variable star
05:53:09.28 +11:49:52.4 -- not a known variable star
05:53:13.27 +14:40:26.4 -- not a known variable star
05:53:16.81 +14:42:25.5 -- not a known variable star
05:53:22.72 +12:06:18.0 -- not a known variable star
05:53:45.05 +15:09:38.0 -- not a known variable star
05:53:45.27 +15:46:35.8 -- not a known variable star
05:53:56.26 +15:51:26.8 -- a known variable star
05:53:57.36 +12:16:41.1 -- a known variable star
05:53:57.38 +15:58:38.5 -- not a known variable star
05:54:00.73 +14:50:42.4 -- not a known variable star
05:54:08.57 +14:53:55.7 -- not a known variable star
05:54:13.85 +13:11:37.5 -- not a known variable star
05:54:14.08 +15:13:42.7 -- a known variable star
05:54:22.03 +15:30:54.7 -- not a known variable star
05:54:24.85 +15:55:48.1 -- not a known variable star
05:54:30.48 +12:57:30.9 -- not a known variable star
05:54:35.46 +12:10:02.2 -- not a known variable star
05:54:41.60 +12:22:48.9 -- not a known variable star
05:54:48.72 +13:47:50.8 -- not a known variable star
05:55:21.81 +15:39:09.6 -- a known variable star
05:55:30.14 +15:07:44.4 -- not a known variable star
05:55:31.07 +15:11:03.3 -- not a known variable star
05:55:42.04 +14:41:21.9 -- not a known variable star
05:55:47.09 +14:33:50.9 -- a known variable star
05:55:47.25 +14:48:04.2 -- not a known variable star
05:55:49.49 +17:04:43.7 -- a known variable star
05:55:50.17 +17:41:15.7 -- not a known variable star
05:55:56.68 +14:38:13.5 -- not a known variable star
05:55:56.95 +15:40:28.5 -- not a known variable star
05:55:57.28 +16:32:15.5 -- a known variable star
05:56:05.78 +17:53:51.3 -- not a known variable star
05:56:21.65 +17:58:16.6 -- not a known variable star
05:56:26.65 +17:40:49.6 -- not a known variable star
05:56:29.76 +15:23:10.1 -- not a known variable star
05:56:30.04 +12:01:33.2 -- a known variable star
05:56:30.45 +15:24:06.3 -- not a known variable star
05:56:30.91 +12:09:19.9 -- not a known variable star
05:56:31.53 +16:33:11.6 -- not a known variable star
05:56:33.25 +15:11:30.2 -- not a known variable star
05:56:38.86 +17:44:21.4 -- not a known variable star
05:56:44.14 +17:00:11.1 -- not a known variable star
05:56:54.46 +15:03:06.2 -- not a known variable star
05:56:56.29 +16:55:37.5 -- not a known variable star
05:57:00.05 +17:55:40.0 -- not a known variable star
05:57:00.14 +13:28:56.4 -- not a known variable star
05:57:11.85 +14:38:51.9 -- not a known variable star
05:57:12.71 +17:39:14.8 -- not a known variable star
05:57:13.12 +12:48:33.4 -- a known variable star
05:57:13.90 +17:30:31.9 -- not a known variable star
05:57:16.62 +12:53:47.2 -- not a known variable star
05:57:25.12 +15:34:07.5 -- not a known variable star
05:57:25.91 +11:32:51.5 -- a known variable star
05:57:32.63 +14:41:17.1 -- not a known variable star
05:57:33.73 +15:38:38.1 -- not a known variable star
05:57:34.57 +11:12:21.5 -- a known variable star
05:57:35.34 +17:58:56.2 -- not a known variable star
05:57:35.77 +15:03:49.6 -- not a known variable star
05:57:38.21 +16:48:12.8 -- not a known variable star
05:57:41.34 +17:40:40.5 -- not a known variable star
05:57:50.52 +15:53:33.9 -- not a known variable star
05:58:03.65 +15:30:43.4 -- not a known variable star
05:58:04.82 +13:32:09.6 -- not a known variable star
05:58:07.88 +17:09:02.1 -- not a known variable star
05:58:09.45 +17:20:40.6 -- not a known variable star
05:58:16.45 +16:05:42.7 -- a known variable star
05:58:18.72 +18:08:55.4 -- a known variable star
05:58:26.34 +15:59:27.6 -- not a known variable star
05:58:27.39 +16:42:25.2 -- not a known variable star
05:58:27.90 +15:59:40.8 -- not a known variable star
05:58:28.09 +17:33:01.5 -- not a known variable star
05:58:48.35 +13:38:11.6 -- not a known variable star
05:58:51.50 +15:39:36.4 -- not a known variable star
05:58:52.31 +13:37:23.5 -- not a known variable star
05:58:55.65 +14:23:33.8 -- not a known variable star
05:58:56.45 +18:06:46.5 -- not a known variable star
05:59:14.13 +16:16:41.1 -- not a known variable star
05:59:16.87 +12:05:09.6 -- not a known variable star
05:59:39.43 +13:09:23.1 -- not a known variable star
05:59:50.35 +16:54:20.2 -- not a known variable star
05:59:52.66 +12:19:21.9 -- a known variable star
05:59:54.86 +17:17:28.4 -- not a known variable star
05:59:56.14 +11:30:33.4 -- not a known variable star
06:00:20.47 +15:32:27.5 -- not a known variable star
06:00:25.20 +16:41:37.4 -- not a known variable star
06:00:30.08 +09:53:10.7 -- not a known variable star
06:00:38.06 +15:37:20.1 -- not a known variable star
06:00:38.99 +15:55:36.4 -- not a known variable star
06:00:53.07 +12:13:41.6 -- not a known variable star
06:00:53.36 +14:53:46.9 -- a known variable star
06:00:54.64 +15:22:19.2 -- not a known variable star
06:00:57.42 +16:27:52.8 -- not a known variable star
06:01:02.76 +13:48:59.6 -- not a known variable star
06:01:17.11 +15:30:04.1 -- not a known variable star
06:01:17.73 +15:06:07.6 -- not a known variable star
06:01:19.57 +15:34:36.3 -- a known variable star
06:01:20.73 +13:05:22.2 -- not a known variable star
06:01:32.19 +16:40:16.4 -- not a known variable star
06:01:32.33 +14:49:01.0 -- a known variable star
06:01:33.58 +16:49:51.0 -- not a known variable star
06:01:34.55 +16:08:07.9 -- not a known variable star
06:01:37.66 +14:43:11.3 -- not a known variable star
06:01:42.15 +16:14:30.0 -- not a known variable star
06:01:56.65 +16:44:38.7 -- not a known variable star
06:02:05.99 +16:03:13.3 -- not a known variable star
06:02:06.73 +15:11:09.4 -- not a known variable star
06:02:07.05 +16:19:41.2 -- not a known variable star
06:02:09.71 +12:11:04.8 -- not a known variable star
06:02:12.33 +12:06:05.4 -- not a known variable star
06:02:12.90 +14:59:52.0 -- not a known variable star
06:02:24.65 +14:17:47.4 -- a known variable star
06:02:32.64 +14:05:00.5 -- not a known variable star
06:02:38.33 +14:07:59.3 -- not a known variable star
06:02:46.01 +11:05:17.8 -- not a known variable star
06:03:03.62 +13:25:03.3 -- not a known variable star
06:03:24.40 +14:38:53.8 -- not a known variable star
06:03:42.69 +13:07:00.2 -- not a known variable star
06:03:45.61 +14:20:46.4 -- not a known variable star
06:03:52.36 +14:59:05.9 -- a known variable star
06:04:04.16 +17:40:32.2 -- not a known variable star
06:04:08.81 +11:12:57.6 -- not a known variable star
06:04:27.92 +16:29:13.6 -- not a known variable star
06:04:53.18 +10:54:04.3 -- a known variable star
06:05:26.55 +12:45:45.3 -- not a known variable star
06:05:27.21 +10:56:04.5 -- not a known variable star
06:05:30.91 +16:17:58.0 -- not a known variable star
06:05:37.30 +17:10:43.6 -- not a known variable star
06:06:01.07 +16:53:34.0 -- not a known variable star
06:06:04.83 +13:40:16.8 -- not a known variable star
06:06:05.08 +13:21:02.4 -- not a known variable star
06:06:13.05 +16:19:25.1 -- not a known variable star
06:06:22.14 +14:21:40.1 -- not a known variable star
06:06:26.73 +10:44:52.7 -- not a known variable star
06:06:27.04 +10:44:01.4 -- not a known variable star
06:06:48.58 +16:40:37.3 -- not a known variable star
06:06:52.06 +15:48:39.0 -- not a known variable star
06:06:58.48 +14:36:07.9 -- not a known variable star
06:07:01.07 +10:58:45.5 -- a known variable star
06:07:05.41 +10:57:47.1 -- not a known variable star
06:07:08.77 +12:32:29.9 -- not a known variable star
06:07:09.47 +16:42:47.4 -- not a known variable star
06:07:20.22 +16:45:35.4 -- not a known variable star
06:07:36.39 +10:59:23.3 -- not a known variable star
06:07:50.05 +12:50:04.1 -- not a known variable star
06:08:01.86 +15:33:58.0 -- not a known variable star
06:08:07.79 +15:55:02.4 -- not a known variable star
06:08:08.32 +14:27:06.1 -- not a known variable star
06:08:41.20 +17:23:37.2 -- not a known variable star
06:08:55.85 +17:07:40.2 -- not a known variable star
06:09:12.84 +15:40:25.5 -- not a known variable star
06:09:15.54 +11:12:53.5 -- not a known variable star
06:09:52.24 +11:19:55.0 -- a known variable star
06:09:55.66 +14:26:06.5 -- not a known variable star
06:10:07.81 +15:00:28.2 -- not a known variable star
06:10:12.01 +17:42:33.7 -- not a known variable star
06:10:14.13 +13:48:21.8 -- not a known variable star
06:10:22.30 +16:14:32.0 -- not a known variable star
06:10:25.17 +16:38:52.0 -- not a known variable star
06:10:28.05 +13:50:01.6 -- a known variable star
06:10:29.67 +16:02:29.5 -- not a known variable star
06:10:30.91 +14:52:41.1 -- not a known variable star
06:10:32.47 +16:29:30.3 -- not a known variable star
06:10:33.18 +17:47:20.1 -- not a known variable star
06:10:33.47 +16:28:35.0 -- not a known variable star
06:10:34.15 +18:09:01.8 -- not a known variable star
06:10:40.74 +15:14:02.4 -- not a known variable star
06:10:46.67 +14:47:19.1 -- not a known variable star
06:10:55.23 +18:14:13.8 -- not a known variable star
06:10:55.69 +15:29:38.5 -- not a known variable star
06:11:05.87 +16:19:10.2 -- not a known variable star
06:11:09.02 +17:31:04.6 -- not a known variable star
06:11:18.41 +14:47:53.9 -- not a known variable star
06:11:23.67 +14:49:43.7 -- not a known variable star
06:11:37.15 +15:28:26.2 -- not a known variable star
06:11:37.59 +13:51:44.9 -- not a known variable star
06:11:38.95 +16:33:10.4 -- not a known variable star
06:11:39.60 +16:27:38.5 -- a known variable star
06:11:44.47 +17:21:10.7 -- not a known variable star
06:11:58.99 +17:22:43.8 -- not a known variable star
06:12:18.19 +15:12:21.7 -- not a known variable star
06:12:20.10 +10:02:03.9 -- not a known variable star
06:12:26.70 +15:00:24.4 -- not a known variable star
06:12:28.10 +15:20:03.5 -- not a known variable star
06:12:29.71 +12:51:00.4 -- a known variable star
06:12:31.18 +15:20:12.7 -- not a known variable star
06:12:49.42 +11:40:07.8 -- not a known variable star
06:12:51.31 +13:17:02.7 -- a known variable star
06:12:57.12 +17:26:20.6 -- a known variable star
06:13:09.91 +18:03:25.5 -- a known variable star
06:13:14.11 +13:29:52.0 -- a known variable star
06:13:16.49 +15:43:24.4 -- a known variable star
06:13:23.68 +17:13:26.6 -- not a known variable star
06:13:27.44 +14:13:52.4 -- a known variable star
06:13:39.34 +15:30:56.7 -- not a known variable star
06:13:48.73 +12:57:35.1 -- not a known variable star
06:13:49.73 +12:47:06.0 -- not a known variable star
06:13:50.87 +14:44:31.4 -- not a known variable star
06:13:51.21 +16:29:05.2 -- not a known variable star
06:13:55.42 +12:05:34.8 -- a known variable star
06:13:58.17 +14:27:25.2 -- not a known variable star
06:14:02.40 +15:01:15.6 -- not a known variable star
06:14:07.62 +18:00:35.3 -- not a known variable star
06:14:08.37 +17:22:59.0 -- not a known variable star
06:14:35.32 +13:49:52.5 -- not a known variable star
06:14:37.25 +16:02:29.7 -- not a known variable star
06:14:38.16 +13:49:46.1 -- a known variable star
06:14:42.27 +15:10:59.5 -- not a known variable star
06:15:20.07 +14:59:21.8 -- not a known variable star
06:15:24.32 +13:24:20.3 -- not a known variable star
06:15:28.00 +14:23:53.4 -- not a known variable star
06:15:38.04 +17:53:12.8 -- not a known variable star
06:15:49.41 +13:13:07.8 -- not a known variable star
06:15:50.93 +17:58:53.9 -- not a known variable star
06:15:51.77 +13:13:57.6 -- not a known variable star
06:15:53.67 +14:10:16.5 -- not a known variable star
06:16:11.26 +14:06:20.4 -- not a known variable star
06:16:19.85 +14:31:16.3 -- not a known variable star
06:16:27.29 +14:57:43.4 -- not a known variable star
06:16:27.36 +16:42:37.2 -- a known variable star
06:16:41.50 +14:25:10.4 -- not a known variable star
06:16:45.41 +15:33:25.8 -- not a known variable star
06:16:49.33 +14:56:25.0 -- not a known variable star
06:16:56.03 +15:17:01.8 -- not a known variable star
06:16:58.71 +18:09:12.0 -- not a known variable star
06:17:11.15 +15:50:14.3 -- a known variable star
06:17:32.29 +16:47:23.0 -- not a known variable star
06:17:35.48 +14:21:38.5 -- not a known variable star
06:17:52.61 +15:42:08.3 -- not a known variable star
06:18:02.62 +17:41:17.8 -- not a known variable star
06:18:06.36 +11:26:20.6 -- not a known variable star
06:18:18.15 +14:22:19.4 -- not a known variable star
06:18:28.87 +14:20:26.5 -- not a known variable star
06:18:42.38 +17:53:59.0 -- a known variable star
06:18:52.50 +13:48:26.1 -- not a known variable star
06:18:53.63 +17:20:32.0 -- not a known variable star
06:18:54.41 +11:33:57.4 -- not a known variable star
06:19:01.55 +14:21:47.0 -- not a known variable star
06:19:02.10 +16:47:08.2 -- not a known variable star
06:19:04.28 +16:47:19.9 -- not a known variable star
06:19:12.12 +12:45:05.8 -- a known variable star
06:19:14.38 +17:25:24.8 -- not a known variable star
06:19:36.65 +17:40:28.7 -- not a known variable star
06:19:42.39 +15:59:26.3 -- not a known variable star
06:19:47.07 +16:38:51.9 -- not a known variable star
06:19:59.31 +17:10:05.9 -- not a known variable star
06:20:00.56 +17:12:18.2 -- not a known variable star
06:20:06.66 +15:51:59.5 -- not a known variable star
06:20:10.22 +12:07:10.0 -- a known variable star
06:20:14.51 +13:20:23.6 -- not a known variable star
06:20:25.32 +17:59:14.9 -- not a known variable star
06:20:25.62 +16:52:34.9 -- not a known variable star
06:20:41.97 +17:05:20.2 -- not a known variable star
06:20:46.12 +17:46:19.4 -- not a known variable star
06:20:46.44 +15:18:14.8 -- not a known variable star
06:20:51.87 +17:05:08.9 -- not a known variable star
06:20:57.18 +16:50:14.0 -- not a known variable star
06:20:58.24 +16:02:33.0 -- not a known variable star
06:20:58.57 +14:41:22.8 -- a known variable star
06:21:19.04 +12:51:49.2 -- not a known variable star
06:21:24.15 +14:10:53.8 -- not a known variable star
06:21:38.01 +12:02:48.8 -- not a known variable star
06:21:43.51 +12:44:21.3 -- not a known variable star
06:22:05.27 +17:47:57.3 -- a known variable star
06:22:11.62 +16:05:21.3 -- not a known variable star
06:23:25.04 +17:30:59.4 -- not a known variable star
06:23:49.23 +16:28:13.4 -- not a known variable star
06:24:13.84 +15:54:30.3 -- not a known variable star
06:25:04.28 +16:36:40.6 -- not a known variable star
06:25:09.44 +15:58:53.2 -- not a known variable star
06:25:19.99 +15:08:17.2 -- not a known variable star
06:25:33.70 +17:35:15.0 -- not a known variable star
06:25:36.63 +13:37:49.9 -- not a known variable star
06:25:40.26 +17:47:38.4 -- not a known variable star
06:25:51.85 +15:01:10.9 -- a known variable star
06:25:55.13 +15:51:16.3 -- not a known variable star
06:25:59.18 +14:56:44.5 -- not a known variable star
06:26:03.55 +16:32:25.5 -- not a known variable star
06:26:05.78 +16:32:36.8 -- not a known variable star
06:26:09.52 +14:11:10.7 -- not a known variable star
06:26:36.81 +17:47:21.7 -- not a known variable star
06:27:07.95 +16:55:01.9 -- not a known variable star
06:27:09.44 +15:25:23.6 -- not a known variable star
06:27:31.24 +15:16:12.7 -- not a known variable star
06:27:44.25 +17:39:43.5 -- not a known variable star
06:27:51.81 +16:41:07.0 -- a known variable star
06:27:52.40 +16:41:35.9 -- not a known variable star
06:27:55.34 +17:41:36.1 -- not a known variable star
06:28:04.93 +14:04:45.4 -- not a known variable star
06:28:32.96 +15:25:10.6 -- not a known variable star
06:28:49.44 +15:22:57.9 -- not a known variable star
06:29:32.69 +17:39:52.8 -- not a known variable star
06:29:40.10 +11:43:01.9 -- not a known variable star
06:29:40.32 +17:17:01.6 -- not a known variable star
06:31:32.15 +18:03:36.5 -- not a known variable star
06:31:42.82 +11:11:14.9 -- not a known variable star
06:32:06.11 +18:09:37.2 -- not a known variable star
06:34:16.98 +17:15:29.9 -- not a known variable star
06:34:47.09 +15:31:01.1 -- not a known variable star
06:35:02.86 +17:42:00.9 -- not a known variable star
06:35:06.77 +12:37:58.3 -- a known variable star
06:35:19.20 +14:30:00.3 -- not a known variable star
06:35:42.69 +11:30:05.7 -- not a known variable star
06:35:48.68 +18:02:11.9 -- not a known variable star
06:36:11.37 +17:16:23.4 -- not a known variable star
06:36:16.00 +17:59:28.7 -- not a known variable star
06:36:29.76 +16:46:34.6 -- not a known variable star
06:37:54.50 +17:30:25.6 -- not a known variable star
06:38:34.20 +17:37:22.6 -- not a known variable star
06:38:45.68 +13:41:32.4 -- not a known variable star
06:38:54.23 +17:47:26.8 -- not a known variable star
06:38:54.79 +15:11:20.6 -- not a known variable star
06:39:09.96 +13:11:14.6 -- not a known variable star
06:39:17.07 +15:47:13.6 -- not a known variable star
06:39:55.14 +13:35:03.6 -- a known variable star
06:40:42.95 +17:09:24.7 -- not a known variable star
06:40:48.75 +17:56:48.8 -- not a known variable star
06:41:08.40 +16:06:36.5 -- not a known variable star
06:41:18.50 +18:02:07.2 -- not a known variable star
06:41:44.73 +15:13:17.5 -- not a known variable star
06:41:51.58 +15:27:19.7 -- a known variable star
Found 308 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
360 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 360 (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)2461128.62294015 -observatory 500
22:51:37.50 -08:08:38.8 Mercury (0.5mag)
01:43:48.15 +10:08:30.6 Venus (-3.9mag)
23:26:44.24 -04:44:01.0 Mars (1.2mag)
07:06:19.31 +22:55:56.9 Jupiter (-2.2mag)
00:21:04.36 -00:02:14.0 Saturn (0.9mag)
03:44:15.15 +19:36:15.9 Uranus (5.8mag)
00:08:25.17 -00:30:45.8 Neptune (7.8mag)
20:32:40.71 -22:52:54.9 Pluto (14.5mag)
09:33:22.91 +16:12:57.4 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Mar 28 22:36 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461128.62294015:
07:06:12.59 +22:56:11.3 Io (5.7mag)
07:06:19.73 +22:55:59.2 Europa (5.8mag)
07:06:00.64 +22:56:36.2 Ganymede (5.2mag)
07:06:52.24 +22:54:59.6 Callisto (6.5mag)
07:10:14.95 +22:52:52.6 Himalia (15.2mag)
07:06:17.02 +22:56:03.4 Thebe (16.1mag)
07:10:00.75 +23:19:21.7 Elara (17.2mag)
07:03:59.47 +23:45:20.0 Pasiphae (17.3mag)
07:14:59.58 +22:51:46.1 Carme (18.4mag)
00:21:12.41 -00:01:59.6 Titan (8.8mag)
00:21:03.45 -00:02:08.9 Rhea (10.1mag)
00:21:22.51 -00:00:04.4 Iapetus (11.5mag)
00:20:59.41 -00:01:48.0 Hyperion (14.8mag)
00:22:53.87 +00:08:20.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 28 22:36 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461128.62294015:
13:53:03.47 +00:00:36.1 JWST
16:24:14.09 +48:29:35.6 Chandra
07:50:31.68 -26:52:19.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 28 22:36 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461128.62294015 -observatory 500
18:41:49.19 -27:50:01.2 14.0mag P/2010 H2 (Vales)
04:55:17.56 -70:34:41.4 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 +08:23:19.2 17.6mag C/2021 G2 (ATLAS)
23:04:36.58 +28:37:25.9 17.0mag C/2022 E2 (ATLAS)
04:09:05.15 +25:31:49.3 15.8mag C/2022 N2 (PANSTARRS)
09:01:28.46 +31:43:26.7 16.1mag C/2022 QE78 (ATLAS)
08:29:46.53 -02:10:49.4 17.2mag C/2022 R6 (PANSTARRS)
18:56:22.30 +16:59:37.9 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:45:14.20 -11:45:42.1 17.6mag P/2023 B1 (PANSTARRS)
09:18:11.04 -14:53:51.1 17.5mag C/2023 F3 (ATLAS)
21:33:14.78 +62:00:02.6 17.4mag C/2023 H5 (Lemmon)
19:30:30.37 -03:33:08.4 14.4mag C/2023 R1 (PANSTARRS)
21:41:43.83 +83:40:00.4 17.8mag C/2023 X2 (Lemmon)
06:13:51.95 +63:40:36.7 16.9mag C/2024 A1 (ATLAS)
04:30:24.74 +10:30:10.0 9.8mag C/2024 E1 (Wierzchos)
16:29:04.36 +03:27:38.4 17.4mag C/2024 G6 (ATLAS)
20:14:06.66 +10:40:27.9 14.8mag C/2024 J3 (ATLAS)
03:11:03.71 -25:15:19.6 16.4mag C/2024 T5 (ATLAS)
05:02:44.85 +50:07:01.5 17.6mag C/2025 J1 (Borisov)
14:48:58.43 +28:10:53.4 14.5mag C/2025 L1 (ATLAS)
02:59:03.47 -23:38:15.3 17.7mag C/2025 Q3 (ATLAS)
22:39:46.43 +19:32:45.6 11.4mag C/2025 R3 (PANSTARRS)
13:01:49.75 +01:51:21.9 17.6mag C/2025 Y1 (ATLAS)
01:44:20.42 -00:58:06.0 11.6mag C/2026 A1 (MAPS)
23:05:37.07 +33:18:45.8 14.0mag C/2026 B2 (Sun-Gao)
18:07:59.49 -10:33:58.8 12.9mag 10P/Tempel
15:21:15.24 +04:40:57.5 12.5mag 24P/Schaumasse
11:08:42.37 -02:10:01.4 15.7mag 29P/Schwassmann-Wachmann
17:51:09.56 -10:19:25.6 17.5mag 40P/Vaisala
10:41:24.58 -05:44:07.9 16.6mag 43P/Wolf-Harrington
01:21:14.16 +14:22:31.3 17.1mag 47P/Ashbrook-Jackson
06:40:16.31 +40:43:36.9 17.1mag 63P/Wild
23:05:27.07 -13:40:55.9 15.7mag 65P/Gunn
03:17:40.82 +14:37:33.6 15.9mag 76P/West-Kohoutek-Ikemura
00:26:43.12 +04:40:18.3 14.5mag 78P/Gehrels
22:06:16.76 -14:33:51.0 14.5mag 88P/Howell
01:21:39.16 +15:37:31.2 15.2mag 93P/Lovas
04:23:17.14 +31:13:14.2 16.4mag 123P/West-Hartley
08:11:32.73 +46:35:57.8 16.2mag 124P/Mrkos
02:06:10.39 +12:18:58.0 16.4mag 128P/Shoemaker-Holt
02:12:51.19 +12:10:14.3 17.4mag 131P/Mueller
23:56:55.25 +06:22:52.1 12.0mag 141P/Machholz
00:07:11.35 -01:42:39.1 12.1mag 141P-A/Machholz
23:02:43.60 -04:49:11.0 15.1mag 141P-D/Machholz
00:12:51.13 -10:20:13.8 15.3mag 162P/SidingSpring
10:34:23.79 +31:52:53.3 17.7mag 164P/Christensen
06:03:53.34 +24:40:04.3 17.7mag 198P/ODAS
15:21:53.66 -02:15:29.4 17.1mag 210P/Christensen
20:41:41.51 -15:44:07.8 17.3mag 218P/LINEAR
17:06:58.13 -15:55:25.7 16.2mag 235P/LINEAR
04:57:13.49 +33:00:05.3 16.5mag 240P/NEAT
07:31:35.49 -07:17:40.4 17.6mag 242P/Spahr
15:47:42.70 +05:42:44.2 17.6mag 391P/Kowalski
07:29:03.46 +21:13:39.6 17.6mag 450P/LONEOS
05:11:06.47 +46:06:04.6 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Mar 28 22:36 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 22:36 asassn_transients_list.txt
############################################################
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 22:36 tocp_transients_list.txt