Mean magnitude and position on the discovery images:
2026 02 27.0800 2461098.5800 13.29 21:16:43.80 +56:56:59.1
96.73955 5.43381 galactic Cep Second-epoch detections are separated by 2.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.1792+56.9482 | 21:16:43.80 +56:56:59.1 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J319.1792+56.9482,2461098.5800,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.1792+56.9482 20260227.0800 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/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:43.80 +56:56:59.1 ;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_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0800 2461098.5800 13.14 21:16:46.72 +56:55:05.4
96.72133 5.40711 galactic Cep Second-epoch detections are separated by 1.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J319.1937+56.9145 | 21:16:46.72 +56:55:05.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.832+/- (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J319.1937+56.9145,2461098.5800,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J319.1937+56.9145 20260227.0800 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/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:16:46.72 +56:55:05.4 ;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_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0800 2461098.5800 12.70 21:17:04.29 +58:29:39.4
97.89030 6.47192 galactic Cep Second-epoch detections are separated by 1.2" and 7.8 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 2191115189971110912 | 21:17:04.16 +58:29:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.125+/-0.025 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2191115189971110912,2461098.5800,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2191115189971110912 20260227.0800 12.70CV 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/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:17:04.29 +58:29:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0800 2461098.5800 11.92 21:29:58.83 +56:59:17.6
98.05359 4.19007 galactic Cep Second-epoch detections are separated by 0.4" and 7.8 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 2178768675127726720 | 21:29:58.74 +56:59:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1958TrRig...7...33A Cl Trumpler 37 134 J-Ks=0.233+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2178768675127726720,2461098.5800,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2178768675127726720 20260227.0800 11.92CV 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/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:29:58.83 +56:59:17.6 ;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_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0800 2461098.5800 12.31 21:17:02.20 +59:13:29.6
98.41779 6.98123 galactic Cep Second-epoch detections are separated by 1.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2191431544374573568 | 21:17:02.05 +59:13:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.118+/-0.028 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2191431544374573568,2461098.5800,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2191431544374573568 20260227.0800 12.31CV 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/Cep-06-Q1b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q1b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-06-Q1b1x1_195605_TTUQ1b1x1_24633_Ih19JuDa/fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20.00sec_-15.00C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:17:02.20 +59:13:29.6 ;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_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-55-23_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q1b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q1b1x1_2026-02-26_19-54-34_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0811 2461098.5811 14.00 00:45:07.32 +55:59:15.1
122.04236 -6.87331 galactic Cas Second-epoch detections are separated by 8.5" and 3.8 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 J011.2799+55.9892 | 00:45:07.32 +55:59:15.1 (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 02 27.0811* 00 45 07.32 +55 59 15.1 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J011.2799+55.9892,2461098.5811,14.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.2799+55.9892 20260227.0811 14.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-04-Q1b1x1_195807_TTUQ1b1x1_945_wAJPusGF/fd_Cas-04-Q1b1x1_2026-02-26_19-56-13_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-04-Q1b1x1_195807_TTUQ1b1x1_945_wAJPusGF/fd_Cas-04-Q1b1x1_2026-02-26_19-57-01_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:07.32 +55:59:15.1 ;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_Cas-04-Q1b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Cas-04-Q1b1x1_2026-02-26_19-57-01_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q1b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Cas-04-Q1b1x1_2026-02-26_19-56-13_20_00sec_-14_90C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q1b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Cas-04-Q1b1x1_2026-02-26_19-57-01_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q1b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Cas-04-Q1b1x1_2026-02-26_19-56-13_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0811* 23 28 13.74 +57 49 30.5 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.5811,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0811 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-22_22-08-57_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-04-Q1b1x1_195807_TTUQ1b1x1_945_wAJPusGF/fd_Cas-04-Q1b1x1_2026-02-26_19-56-13_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-04-Q1b1x1_195807_TTUQ1b1x1_945_wAJPusGF/fd_Cas-04-Q1b1x1_2026-02-26_19-57-01_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:28:13.74 +57:49:30.5 ;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_Cas-04-Q1b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Cas-04-Q1b1x1_2026-02-26_19-57-01_20_00sec_-15_00C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-04-Q1b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Cas-04-Q1b1x1_2026-02-26_19-56-13_20_00sec_-14_90C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q1b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Cas-04-Q1b1x1_2026-02-26_19-57-01_20_00sec_-15_00C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-04-Q1b1x1_2025-12-22_22-08-57_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Cas-04-Q1b1x1_2026-02-26_19-56-13_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0870* 01 16 55.18 +55 37 02.7 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.5870,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0870 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/Cas-05-Q1b1x1_2025-12-22_23-12-51_20.00sec_-15.00C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-05-Q1b1x1_200620_TTUQ1b1x1_8602_4qJFjf7J/fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-05-Q1b1x1_200620_TTUQ1b1x1_8602_4qJFjf7J/fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:16:55.18 +55:37:02.7 ;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_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0870 2461098.5870 13.72 00:36:38.83 +49:23:23.1
120.45853 -13.41095 galactic Cas Second-epoch detections are separated by 2.6" and 1.9 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 391416351262088448 | 00:36:40.77 +49:23:47.7 (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 02 27.0870* 00 36 38.83 +49 23 23.1 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391416351262088448,2461098.5870,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 391416351262088448 20260227.0870 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/Cas-05-Q1b1x1_2025-12-22_23-12-51_20.00sec_-15.00C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-05-Q1b1x1_200620_TTUQ1b1x1_8602_4qJFjf7J/fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-05-Q1b1x1_200620_TTUQ1b1x1_8602_4qJFjf7J/fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:38.83 +49:23:23.1 ;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_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0870* 00 54 18.13 +51 09 04.5 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.5870,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0870 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/Cas-05-Q1b1x1_2025-12-22_23-12-51_20.00sec_-15.00C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-05-Q1b1x1_200620_TTUQ1b1x1_8602_4qJFjf7J/fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-05-Q1b1x1_200620_TTUQ1b1x1_8602_4qJFjf7J/fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:54:18.13 +51:09:04.5 ;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_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0870* 01 50 54.45 +48 46 54.2 14.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015053.78+484711.9,2461098.5870,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015053.78+484711.9 20260227.0870 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/Cas-05-Q1b1x1_2025-12-22_23-12-51_20.00sec_-15.00C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-05-Q1b1x1_200620_TTUQ1b1x1_8602_4qJFjf7J/fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-05-Q1b1x1_200620_TTUQ1b1x1_8602_4qJFjf7J/fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:50:54.45 +48:46:54.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-05-20_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-05-Q1b1x1_2025-12-22_23-12-51_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png resample_wcs_fd_Cas-05-Q1b1x1_2026-02-26_20-04-44_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0855 2461098.5855 13.22 07:46:12.82 -22:26:13.7
239.00718 1.18650 galactic Pup Second-epoch detections are separated by 0.7" and 6.3 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 J116.5519-22.4335 | 07:46:12.92 -22:25:32.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.232+/-0.064 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J116.5519-22.4335,2461098.5855,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J116.5519-22.4335 20260227.0855 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-02-Q1b1x1_200423_TTUQ1b1x1_13847_nMqwqYOT/fd_Pup-02-Q1b1x1_2026-02-26_20-02-26_20.00sec_-15.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-02-Q1b1x1_200423_TTUQ1b1x1_13847_nMqwqYOT/fd_Pup-02-Q1b1x1_2026-02-26_20-03-32_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:12.82 -22:26:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-02-Q1b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q1b1x1_2026-02-26_20-03-32_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q1b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q1b1x1_2026-02-26_20-02-26_20_00sec_-15_00C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q1b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q1b1x1_2026-02-26_20-03-32_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q1b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q1b1x1_2026-02-26_20-02-26_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
ASAS J072910-2653.3,2461098.5855,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J072910-2653.3 20260227.0855 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-01-08_23-27-09_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-02-Q1b1x1_2026-01-08_23-27-45_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-02-Q1b1x1_200423_TTUQ1b1x1_13847_nMqwqYOT/fd_Pup-02-Q1b1x1_2026-02-26_20-02-26_20.00sec_-15.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-02-Q1b1x1_200423_TTUQ1b1x1_13847_nMqwqYOT/fd_Pup-02-Q1b1x1_2026-02-26_20-03-32_20.00sec_-15.00C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:29:10.43 -26:53:22.2 ;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_Pup-02-Q1b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q1b1x1_2026-02-26_20-03-32_20_00sec_-15_00C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-02-Q1b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q1b1x1_2026-02-26_20-02-26_20_00sec_-15_00C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q1b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q1b1x1_2026-02-26_20-03-32_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-02-Q1b1x1_2026-01-08_23-27-09_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_fd_Pup-02-Q1b1x1_2026-02-26_20-02-26_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0839* 00 20 24.47 +62 23 55.6 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J002022.21+622409.7,2461098.5839,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J002022.21+622409.7 20260227.0839 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-02-Q1b1x1_200226_TTUQ1b1x1_19467_YdWtrSVR/fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-02-Q1b1x1_200226_TTUQ1b1x1_19467_YdWtrSVR/fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20.00sec_-14.90C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:20:24.47 +62:23:55.6 ;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_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20_00sec_-14_90C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20_00sec_-14_90C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0839 2461098.5839 13.34 22:59:10.55 +58:14:26.3
108.58925 -1.47011 galactic Cas Second-epoch detections are separated by 2.8" and 6.3 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 J344.7948+58.2380 | 22:59:07.86 +58:14:15.5 (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 02 27.0839* 22 59 10.55 +58 14 26.3 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J344.7948+58.2380,2461098.5839,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J344.7948+58.2380 20260227.0839 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-02-Q1b1x1_200226_TTUQ1b1x1_19467_YdWtrSVR/fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-02-Q1b1x1_200226_TTUQ1b1x1_19467_YdWtrSVR/fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20.00sec_-14.90C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:59:10.55 +58:14:26.3 ;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_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20_00sec_-14_90C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20_00sec_-14_90C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0839* 00 57 22.97 +60 19 40.1 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.5839,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0839 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-02-Q1b1x1_200226_TTUQ1b1x1_19467_YdWtrSVR/fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-02-Q1b1x1_200226_TTUQ1b1x1_19467_YdWtrSVR/fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20.00sec_-14.90C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:57:22.97 +60:19:40.1 ;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_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20_00sec_-14_90C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20_00sec_-14_90C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0839 2461098.5839 13.80 00:50:46.77 +56:37:02.2
122.84080 -6.25435 galactic Cas Second-epoch detections are separated by 3.3" and 6.5 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 J012.6886+56.6234 | 00:50:43.05 +56:37:19.3 (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 02 27.0839* 00 50 46.77 +56 37 02.2 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J012.6886+56.6234,2461098.5839,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012.6886+56.6234 20260227.0839 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-02-Q1b1x1_200226_TTUQ1b1x1_19467_YdWtrSVR/fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-02-Q1b1x1_200226_TTUQ1b1x1_19467_YdWtrSVR/fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20.00sec_-14.90C_LIGHT_0011.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:50:46.77 +56:37:02.2 ;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_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20_00sec_-14_90C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20_00sec_-15_00C_LIGHT_0010_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-01-02_20_00sec_-14_90C_LIGHT_0011_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-02-26_20-00-14_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0904* 01 59 10.44 +56 41 33.6 14.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 504876502326747904,2461098.5904,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 504876502326747904 20260227.0904 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/Cas-03-Q1b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:10.44 +56:41:33.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0904 2461098.5904 13.35 01:29:42.69 +60:58:11.6
127.56035 -1.55745 galactic Cas Second-epoch detections are separated by 1.7" and 6.7 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 510636568868023168 | 01:29:38.75 +60:58:44.3 (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 02 27.0904* 01 29 42.69 +60 58 11.6 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510636568868023168,2461098.5904,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510636568868023168 20260227.0904 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/Cas-03-Q1b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:29:42.69 +60:58:11.6 ;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_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0904* 02 16 37.35 +64 56 47.0 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 515428274899734784,2461098.5904,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 515428274899734784 20260227.0904 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/Cas-03-Q1b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:16:37.35 +64:56:47.0 ;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_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0904 2461098.5904 14.02 02:04:36.16 +58:50:58.3
132.28555 -2.68713 galactic Per Second-epoch detections are separated by 2.9" and 6.6 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 J031.1552+58.8491 | 02:04:36.16 +58:50:58.3 (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 02 27.0904* 02 04 36.16 +58 50 58.3 14.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J031.1552+58.8491,2461098.5904,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J031.1552+58.8491 20260227.0904 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/Cas-03-Q1b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:36.16 +58:50:58.3 ;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_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0904* 02 18 52.28 +62 48 14.2 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1867220,2461098.5904,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1867220 20260227.0904 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/Cas-03-Q1b1x1_2025-12-22_23-38-59_20.00sec_-14.90C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2025-12-22_23-39-45_20.00sec_-15.00C_LIGHT_0253.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-03-Q1b1x1_201105_TTUQ1b1x1_25367_eMXQ3rTM/fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:18:52.28 +62:48:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-10-27_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-03-Q1b1x1_2025-12-22_23-38-59_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png resample_wcs_fd_Cas-03-Q1b1x1_2026-02-26_20-09-30_20_00sec_-15_00C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 5538493682643041536,2461098.5824,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5538493682643041536 20260227.0824 11.05CV 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/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:52:06.78 -38:35:08.9 ;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_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0824 2461098.5824 13.45 07:51:37.84 -29:10:15.3
245.43060 -1.17418 galactic Pup Second-epoch detections are separated by 3.7" and 1.4 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 J117.9077-29.1691 | 07:51:37.84 -29:10:15.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J117.9077-29.1691,2461098.5824,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J117.9077-29.1691 20260227.0824 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/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:37.84 -29:10:15.3 ;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_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0824 2461098.5824 13.13 07:35:34.89 -31:11:04.3
245.45950 -5.18424 galactic Pup Second-epoch detections are separated by 3.4" and 1.3 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 J113.8962-31.1908 | 07:35:36.38 -31:10:54.1 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 J113.8962-31.1908,2461098.5824,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J113.8962-31.1908 20260227.0824 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/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:35:34.89 -31:11:04.3 ;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_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0824 2461098.5824 13.44 07:11:05.50 -29:52:30.1
241.84532 -9.26678 galactic CMa Second-epoch detections are separated by 3.9" and 1.3 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 | ASAS J071106-2952.1 | 07:11:06.24 -29:52:02.7 (Gaia DR3) | MISC (local) | 2452197.40000 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J071106-2952.1,2461098.5824,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J071106-2952.1 20260227.0824 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:05.50 -29:52:30.1 ;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_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 5598006261324780544,2461098.5824,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5598006261324780544 20260227.0824 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/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:40:43.77 -32:17:31.3 ;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_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0824 2461098.5824 13.35 06:38:43.32 -38:14:09.6
247.03041 -18.72194 galactic Col Second-epoch detections are separated by 3.7" and 0.6 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 | 06:38:43.32 -38:14:09.6 (user input) | T | P | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0824* 06 38 43.32 -38 14 09.6 13.3 U Col 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.5824,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0824 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/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:38:43.32 -38:14:09.6 ;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_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0824 2461098.5824 13.61 07:44:03.86 -35:34:13.8
250.17469 -5.76650 galactic Pup Second-epoch detections are separated by 2.6" and 1.0 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 5587666965068444544 | 07:44:05.64 -35:34:54.1 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 5587666965068444544,2461098.5824,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5587666965068444544 20260227.0824 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/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:44:03.86 -35:34:13.8 ;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_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0824 2461098.5824 13.66 07:17:41.84 -30:02:38.4
242.64185 -8.06033 galactic CMa Second-epoch detections are separated by 5.0" and 1.4 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 5606045168791232640 | 07:17:42.50 -30:02:07.4 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 5606045168791232640,2461098.5824,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5606045168791232640 20260227.0824 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/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:17:41.84 -30:02:38.4 ;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_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.5824,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0824 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/Pup-03-Q1b1x1_2026-01-20_21-47-37_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20.00sec_-15.00C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-03-Q1b1x1_200022_TTUQ1b1x1_13870_4EorhEXe/fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20.00sec_-14.90C_LIGHT_0009.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:06:20.17 -29:49:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-47_20_00sec_-14_90C_LIGHT_0009_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-03-Q1b1x1_2026-01-20_21-47-37_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png resample_wcs_fd_Pup-03-Q1b1x1_2026-02-26_19-58-12_20_00sec_-15_00C_LIGHT_0008_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0944 2461098.5944 12.76 01:10:20.01 +66:06:35.9
124.84639 3.30849 galactic Cas Second-epoch detections are separated by 4.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | V0891 Cas | 01:10:22.29 +66:07:12.5 (Gaia DR3) | SR (local) | 232.444293100000 (local) | Gaia3var=VARIABLE SpType: M7 1980PW&SO...2f...1B IRC +70018
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0944* 01 10 20.01 +66 06 35.9 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0891 Cas,2461098.5944,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0891 Cas 20260227.0944 12.76CV 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-03-Q1b1x1_201650_TTUQ1b1x1_30563_XoExfMbp/fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-03-Q1b1x1_201650_TTUQ1b1x1_30563_XoExfMbp/fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20.00sec_-15.00C_LIGHT_0026.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:10:20.01 +66:06:35.9 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20_00sec_-15_00C_LIGHT_0026_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20_00sec_-15_00C_LIGHT_0025_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20_00sec_-15_00C_LIGHT_0025_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0944* 23 52 09.49 +65 39 06.8 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.5944,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0944 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-03-Q1b1x1_201650_TTUQ1b1x1_30563_XoExfMbp/fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-03-Q1b1x1_201650_TTUQ1b1x1_30563_XoExfMbp/fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20.00sec_-15.00C_LIGHT_0026.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:52:09.49 +65:39:06.8 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20_00sec_-15_00C_LIGHT_0026_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20_00sec_-15_00C_LIGHT_0025_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20_00sec_-15_00C_LIGHT_0025_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0944* 01 22 38.11 +71 09 29.1 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.5944,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0944 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-03-Q1b1x1_201650_TTUQ1b1x1_30563_XoExfMbp/fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-03-Q1b1x1_201650_TTUQ1b1x1_30563_XoExfMbp/fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20.00sec_-15.00C_LIGHT_0026.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:22:38.11 +71:09:29.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20_00sec_-15_00C_LIGHT_0026_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20_00sec_-15_00C_LIGHT_0025_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-16-07_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-02-26_20-15-28_20_00sec_-15_00C_LIGHT_0025_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0915 2461098.5915 14.02 02:21:52.71 +52:44:40.0
136.51600 -7.72548 galactic Per Second-epoch detections are separated by 0.4" and 7.1 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 J035.4737+52.7432 | 02:21:52.71 +52:44:40.0 (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 02 27.0915* 02 21 52.71 +52 44 40.0 14.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.4737+52.7432,2461098.5915,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J035.4737+52.7432 20260227.0915 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/Per-01-Q1b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q1b1x1_201235_TTUQ1b1x1_31872_VroKcuVR/fd_Per-01-Q1b1x1_2026-02-26_20-11-14_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q1b1x1_201235_TTUQ1b1x1_31872_VroKcuVR/fd_Per-01-Q1b1x1_2026-02-26_20-11-56_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:21:52.71 +52:44:40.0 ;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_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-02-26_20-11-56_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-02-26_20-11-14_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-02-26_20-11-56_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-02-26_20-11-14_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0915 2461098.5915 14.04 02:23:31.09 +52:41:28.7
136.76956 -7.68883 galactic Per Second-epoch detections are separated by 3.5" and 6.6 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 J035.8700+52.6900 | 02:23:31.09 +52:41:28.7 (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 02 27.0915* 02 23 31.09 +52 41 28.7 14.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.8700+52.6900,2461098.5915,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J035.8700+52.6900 20260227.0915 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/Per-01-Q1b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q1b1x1_201235_TTUQ1b1x1_31872_VroKcuVR/fd_Per-01-Q1b1x1_2026-02-26_20-11-14_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-01-Q1b1x1_201235_TTUQ1b1x1_31872_VroKcuVR/fd_Per-01-Q1b1x1_2026-02-26_20-11-56_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:23:31.09 +52:41:28.7 ;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_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-02-26_20-11-56_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-02-26_20-11-14_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-02-26_20-11-56_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-02-26_20-11-14_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0973 2461098.5973 13.46 08:24:52.59 -14:51:23.1
237.35480 12.95419 galactic Pup Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J126.2177-14.8564 | 08:24:52.59 -14:51:23.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J126.2177-14.8564,2461098.5973,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J126.2177-14.8564 20260227.0973 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-01-Q1b1x1_202050_TTUQ1b1x1_20659_S4Zg8VAB/fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-01-Q1b1x1_202050_TTUQ1b1x1_20659_S4Zg8VAB/fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:52.59 -14:51:23.1 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0973 2461098.5973 13.49 08:18:03.18 -16:52:21.4
238.17401 10.48156 galactic Pup Second-epoch detections are separated by 5.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J124.5088-16.8695 | 08:18:03.18 -16:52:21.4 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J124.5088-16.8695,2461098.5973,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J124.5088-16.8695 20260227.0973 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-01-Q1b1x1_202050_TTUQ1b1x1_20659_S4Zg8VAB/fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-01-Q1b1x1_202050_TTUQ1b1x1_20659_S4Zg8VAB/fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:18:03.18 -16:52:21.4 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
MU Pup,2461098.5973,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MU Pup 20260227.0973 12.69CV 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/reference_imgs/Pup-01-Q1b1x1_2025-12-23_01-23-30_20.00sec_-15.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-01-Q1b1x1_202050_TTUQ1b1x1_20659_S4Zg8VAB/fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pup-01-Q1b1x1_202050_TTUQ1b1x1_20659_S4Zg8VAB/fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:54:08.02 -16:47:28.7 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-20-15_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-02-26_20-19-30_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0988 2461098.5988 13.82 02:43:32.49 +57:11:29.5
137.69487 -2.43170 galactic Per Second-epoch detections are separated by 2.3" and 7.2 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 J040.9091+57.1754 | 02:43:35.27 +57:11:00.6 (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 02 27.0988* 02 43 32.49 +57 11 29.5 13.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J040.9091+57.1754,2461098.5988,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J040.9091+57.1754 20260227.0988 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/Cam-08-Q1b1x1_2025-12-23_00-44-54_20.00sec_-14.90C_LIGHT_0330.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-08-Q1b1x1_202305_TTUQ1b1x1_30322_vdHa83iE/fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-08-Q1b1x1_202305_TTUQ1b1x1_30322_vdHa83iE/fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20.00sec_-15.00C_LIGHT_0032.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:43:32.49 +57:11:29.5 ;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_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20_00sec_-15_00C_LIGHT_0032_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0988 2461098.5988 13.88 02:43:10.04 +58:52:25.9
136.94678 -0.92386 galactic Cas Second-epoch detections are separated by 4.3" and 6.4 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 J040.7898+58.8720 | 02:43:10.04 +58:52:25.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.635+/-0.098 (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 02 27.0988* 02 43 10.04 +58 52 25.9 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J040.7898+58.8720,2461098.5988,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J040.7898+58.8720 20260227.0988 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/Cam-08-Q1b1x1_2025-12-23_00-44-54_20.00sec_-14.90C_LIGHT_0330.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-08-Q1b1x1_202305_TTUQ1b1x1_30322_vdHa83iE/fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-08-Q1b1x1_202305_TTUQ1b1x1_30322_vdHa83iE/fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20.00sec_-15.00C_LIGHT_0032.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:43:10.04 +58:52:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20_00sec_-15_00C_LIGHT_0032_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0988* 02 25 28.75 +62 00 33.9 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.5988,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0988 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q1b1x1_2025-12-23_00-44-54_20.00sec_-14.90C_LIGHT_0330.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-08-Q1b1x1_202305_TTUQ1b1x1_30322_vdHa83iE/fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-08-Q1b1x1_202305_TTUQ1b1x1_30322_vdHa83iE/fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20.00sec_-15.00C_LIGHT_0032.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:25:28.75 +62:00:33.9 ;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_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20_00sec_-15_00C_LIGHT_0032_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
GG Cam,2461098.5988,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GG Cam 20260227.0988 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q1b1x1_2025-12-23_00-44-54_20.00sec_-14.90C_LIGHT_0330.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-08-Q1b1x1_2025-12-23_00-45-33_20.00sec_-15.00C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-08-Q1b1x1_202305_TTUQ1b1x1_30322_vdHa83iE/fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-08-Q1b1x1_202305_TTUQ1b1x1_30322_vdHa83iE/fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20.00sec_-15.00C_LIGHT_0032.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:40.92 +61:05:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20_00sec_-15_00C_LIGHT_0032_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20_00sec_-15_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-22-25_20_00sec_-15_00C_LIGHT_0032_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-02-26_20-21-40_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0957* 03 17 03.79 +41 37 53.2 13.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.5957,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0957 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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20.00sec_-15.00C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:17:03.79 +41:37:53.2 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0957 2461098.5957 13.81 03:03:43.97 +48:15:29.4
144.51474 -8.99163 galactic Per Second-epoch detections are separated by 4.0" and 8.6 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 J045.9288+48.2640 | 03:03:43.97 +48:15:29.4 (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 02 27.0957* 03 03 43.97 +48 15 29.4 13.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J045.9288+48.2640,2461098.5957,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J045.9288+48.2640 20260227.0957 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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20.00sec_-15.00C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:43.97 +48:15:29.4 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0957 2461098.5957 14.21 03:29:31.22 +45:23:50.5
149.83491 -9.05696 galactic Per Second-epoch detections are separated by 8.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J052.3685+45.3904 | 03:29:31.22 +45:23:50.5 (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 02 27.0957* 03 29 31.22 +45 23 50.5 14.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J052.3685+45.3904,2461098.5957,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J052.3685+45.3904 20260227.0957 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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20.00sec_-15.00C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:31.22 +45:23:50.5 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0957 2461098.5957 14.27 03:43:28.43 +41:53:28.1
154.01003 -10.36962 galactic Per Second-epoch detections are separated by 1.5" and 8.4 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 J055.8677+41.8931 | 03:43:28.43 +41:53:28.1 (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 02 27.0957* 03 43 28.43 +41 53 28.1 14.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J055.8677+41.8931,2461098.5957,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J055.8677+41.8931 20260227.0957 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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20.00sec_-15.00C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:28.43 +41:53:28.1 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.0957* 03 11 40.87 +41 38 46.8 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GG Per,2461098.5957,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GG Per 20260227.0957 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/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-02-Q1b1x1_201850_TTUQ1b1x1_15196_dzyAfYoi/fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20.00sec_-15.00C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:40.87 +41:38:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-18-05_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-02-26_20-17-18_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1000* 01 45 58.07 +71 41 34.2 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 534325684320188544,2461098.6000,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 534325684320188544 20260227.1000 12.60CV 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/Cas-01-Q1b1x1_2025-12-23_00-01-41_20.00sec_-15.00C_LIGHT_0280.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-01-Q1b1x1_202450_TTUQ1b1x1_27892_nXOgRfKo/fd_Cas-01-Q1b1x1_2026-02-26_20-23-28_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cas-01-Q1b1x1_202450_TTUQ1b1x1_27892_nXOgRfKo/fd_Cas-01-Q1b1x1_2026-02-26_20-24-10_20.00sec_-14.90C_LIGHT_0034.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:58.07 +71:41:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-01-Q1b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q1b1x1_2026-02-26_20-24-10_20_00sec_-14_90C_LIGHT_0034_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-01-Q1b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q1b1x1_2026-02-26_20-23-28_20_00sec_-15_00C_LIGHT_0033_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-01-Q1b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q1b1x1_2026-02-26_20-24-10_20_00sec_-14_90C_LIGHT_0034_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-01-Q1b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q1b1x1_2026-02-26_20-23-28_20_00sec_-15_00C_LIGHT_0033_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6054,9.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1054 9.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-06-Q1b1x1_203250_TTUQ1b1x1_30202_rns9rzyE/fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-06-Q1b1x1_203250_TTUQ1b1x1_30202_rns9rzyE/fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20.00sec_-14.90C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:36:24.36 +03:42:54.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20_00sec_-14_90C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20_00sec_-14_90C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6054,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1054 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-06-Q1b1x1_203250_TTUQ1b1x1_30202_rns9rzyE/fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-06-Q1b1x1_203250_TTUQ1b1x1_30202_rns9rzyE/fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20.00sec_-14.90C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:01:02.18 +06:52:34.0 ;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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20_00sec_-14_90C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20_00sec_-14_90C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6054,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1054 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/Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-06-Q1b1x1_203250_TTUQ1b1x1_30202_rns9rzyE/fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-06-Q1b1x1_203250_TTUQ1b1x1_30202_rns9rzyE/fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20.00sec_-14.90C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:52:40.59 +07:40:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20_00sec_-14_90C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20_00sec_-14_90C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6054,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1054 12.77CV 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/Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-06-Q1b1x1_203250_TTUQ1b1x1_30202_rns9rzyE/fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20.00sec_-14.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-06-Q1b1x1_203250_TTUQ1b1x1_30202_rns9rzyE/fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20.00sec_-14.90C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:07.39 +06:31:15.6 ;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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20_00sec_-14_90C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20_00sec_-14_90C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-32-10_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-02-26_20-30-58_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1118 2461098.6118 12.89 00:30:09.76 +25:04:20.5
116.85282 -37.54813 galactic And Second-epoch detections are separated by 1.4" and 7.8 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 | 00:30:09.76 +25:04:20.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.628+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1118* 00 30 09.76 +25 04 20.5 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6118,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1118 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/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-01-Q1b1x1_204150_TTUQ1b1x1_17334_k2WbgPos/fd_Psc-01-Q1b1x1_2026-02-26_20-40-22_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-01-Q1b1x1_204150_TTUQ1b1x1_17334_k2WbgPos/fd_Psc-01-Q1b1x1_2026-02-26_20-41-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:09.76 +25:04:20.5 ;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_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-26_20-41-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-26_20-40-22_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-26_20-41-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-26_20-40-22_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6131,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1131 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20.00sec_-15.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:12.77 +17:29:26.8 ;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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6131,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1131 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/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20.00sec_-15.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:37:26.74 +13:59:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6131,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1131 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/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20.00sec_-15.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:42.68 +16:42:17.2 ;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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1131* 01 48 34.18 +12 07 05.2 13.9 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6131,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1131 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/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20.00sec_-15.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:34.18 +12:07:05.2 ;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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1131* 01 59 23.51 +10 42 45.5 14.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6131,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1131 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/Psc-03-Q1b1x1_2025-12-22_22-40-30_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20.00sec_-15.00C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Psc-03-Q1b1x1_204350_TTUQ1b1x1_4141_S0FXBi9c/fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:23.51 +10:42:45.5 ;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_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-43-08_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-03-Q1b1x1_2025-12-22_22-40-30_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png resample_wcs_fd_Psc-03-Q1b1x1_2026-02-26_20-42-16_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1197 2461098.6197 11.41 01:04:35.61 +41:17:57.9
125.58713 -21.50450 galactic And Second-epoch detections are separated by 0.2" and 4.9 pix This object is listed in neverexclude_list.txt 0.8" RX And - radio detected CVThe object was found in VSX 1" RX And
Type: UGZ
# Max. Min./Amp. JD0 Period
10.300 V 14.800 V 0.209893000000 pec(UG)
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1197* 01 04 35.61 +41 17 57.9 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RX And,2461098.6197,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX And 20260227.1197 11.41CV 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/And-05-Q1b1x1_2025-12-22_22-44-00_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-05-Q1b1x1_205305_TTUQ1b1x1_4293_ZLBT1aFK/fd_And-05-Q1b1x1_2026-02-26_20-51-48_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-05-Q1b1x1_205305_TTUQ1b1x1_4293_ZLBT1aFK/fd_And-05-Q1b1x1_2026-02-26_20-52-29_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:04:35.61 +41:17:57.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-05-Q1b1x1_2025-12-22_22-44-00_20_00sec_-14_90C_LIGHT_0192_fits__*pix.png resample_wcs_fd_And-05-Q1b1x1_2026-02-26_20-52-29_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-05-Q1b1x1_2025-12-22_22-44-00_20_00sec_-14_90C_LIGHT_0192_fits__*pix.png resample_wcs_fd_And-05-Q1b1x1_2026-02-26_20-51-48_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-05-Q1b1x1_2025-12-22_22-44-00_20_00sec_-14_90C_LIGHT_0192_fits__*pix.png resample_wcs_fd_And-05-Q1b1x1_2026-02-26_20-52-29_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-05-Q1b1x1_2025-12-22_22-44-00_20_00sec_-14_90C_LIGHT_0192_fits__*pix.png resample_wcs_fd_And-05-Q1b1x1_2026-02-26_20-51-48_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1197 2461098.6197 11.39 01:04:35.58 +41:17:58.3
125.58702 -21.50439 galactic And Second-epoch detections are separated by 0.3" and 4.8 pix This object is listed in neverexclude_list.txt 0.7" RX And - radio detected CVThe object was found in VSX 1" RX And
Type: UGZ
# Max. Min./Amp. JD0 Period
10.300 V 14.800 V 0.209893000000 pec(UG)
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1197* 01 04 35.58 +41 17 58.3 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RX And,2461098.6197,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX And 20260227.1197 11.39CV 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/And-05-Q1b1x1_2025-12-22_22-44-00_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/reference_imgs/And-05-Q1b1x1_2025-12-22_22-44-55_20.00sec_-15.00C_LIGHT_0193.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-05-Q1b1x1_205305_TTUQ1b1x1_4293_ZLBT1aFK/fd_And-05-Q1b1x1_2026-02-26_20-51-48_20.00sec_-15.00C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-05-Q1b1x1_205305_TTUQ1b1x1_4293_ZLBT1aFK/fd_And-05-Q1b1x1_2026-02-26_20-52-29_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:04:35.58 +41:17:58.3 ;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_And-05-Q1b1x1_2025-12-22_22-44-00_20_00sec_-14_90C_LIGHT_0192_fits__*pix.png resample_wcs_fd_And-05-Q1b1x1_2026-02-26_20-52-29_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-05-Q1b1x1_2025-12-22_22-44-00_20_00sec_-14_90C_LIGHT_0192_fits__*pix.png resample_wcs_fd_And-05-Q1b1x1_2026-02-26_20-51-48_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-05-Q1b1x1_2025-12-22_22-44-00_20_00sec_-14_90C_LIGHT_0192_fits__*pix.png resample_wcs_fd_And-05-Q1b1x1_2026-02-26_20-52-29_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-05-Q1b1x1_2025-12-22_22-44-00_20_00sec_-14_90C_LIGHT_0192_fits__*pix.png resample_wcs_fd_And-05-Q1b1x1_2026-02-26_20-51-48_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,2461098.6208,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1208 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/Ari-02-Q1b1x1_2025-12-22_22-54-34_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-02-Q1b1x1_205450_TTUQ1b1x1_19939_iUfZfPiq/fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20.00sec_-14.90C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-02-Q1b1x1_205450_TTUQ1b1x1_19939_iUfZfPiq/fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20.00sec_-14.90C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:13.81 +17:29:30.4 ;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_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20_00sec_-14_90C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20_00sec_-14_90C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20_00sec_-14_90C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1209* 01 58 24.30 +22 11 01.8 13.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6208,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1208 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/Ari-02-Q1b1x1_2025-12-22_22-54-34_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-02-Q1b1x1_205450_TTUQ1b1x1_19939_iUfZfPiq/fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20.00sec_-14.90C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-02-Q1b1x1_205450_TTUQ1b1x1_19939_iUfZfPiq/fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20.00sec_-14.90C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:58:24.30 +22:11:01.8 ;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_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20_00sec_-14_90C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20_00sec_-14_90C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20_00sec_-14_90C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1209* 01 58 09.59 +22 08 32.0 13.8 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6208,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1208 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/Ari-02-Q1b1x1_2025-12-22_22-54-34_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-02-Q1b1x1_205450_TTUQ1b1x1_19939_iUfZfPiq/fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20.00sec_-14.90C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-02-Q1b1x1_205450_TTUQ1b1x1_19939_iUfZfPiq/fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20.00sec_-14.90C_LIGHT_0062.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:58:09.59 +22:08:32.0 ;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_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20_00sec_-14_90C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20_00sec_-14_90C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-54-09_20_00sec_-14_90C_LIGHT_0062_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-02-Q1b1x1_2025-12-22_22-54-34_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png resample_wcs_fd_Ari-02-Q1b1x1_2026-02-26_20-53-32_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 02 32 19.11 +08 30 56.3 13.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6218,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1218 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:19.11 +08:30:56.3 ;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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 02 45 26.48 +07 46 12.1 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6218,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1218 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:45:26.48 +07:46:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 02 07 10.91 +01 09 59.2 13.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6218,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1218 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:10.91 +01:09:59.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 03 04 23.71 +07 39 38.8 14.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6218,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1218 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:04:23.71 +07:39:38.8 ;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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 02 59 36.52 +10 53 32.1 14.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.6218,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1218 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:36.52 +10:53:32.1 ;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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 03 00 30.02 +08 57 51.4 14.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6218,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1218 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:30.02 +08:57:51.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 2948040026990248320,2461098.5930,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2948040026990248320 20260227.0930 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20.00sec_-14.90C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:57:26.98 -15:24:27.9 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.0930 2461098.5930 13.51 07:14:09.78 -22:39:57.9
235.65920 -5.41786 galactic CMa Second-epoch detections are separated by 1.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.5630-22.6614 | 07:14:12.86 -22:39:48.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.5630-22.6614,2461098.5930,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J108.5630-22.6614 20260227.0930 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20.00sec_-14.90C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:09.78 -22:39:57.9 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.5930,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.0930 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20.00sec_-14.90C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:48.01 -19:25:18.0 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
ASAS J065945-1421.1,2461098.5930,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J065945-1421.1 20260227.0930 12.58CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20.00sec_-14.90C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:44.77 -14:21:11.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
BP CMa,2461098.5930,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BP CMa 20260227.0930 12.09CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-02-Q1b1x1_201450_TTUQ1b1x1_8110_sVnjFR0x/fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20.00sec_-14.90C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:15:19.68 -22:00:43.8 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-14-05_20_00sec_-14_90C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-02-26_20-13-20_20_00sec_-15_00C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1259 2461098.6259 13.32 06:59:18.54 -21:11:00.4
232.77024 -7.83249 galactic CMa Second-epoch detections are separated by 2.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.8395-21.1845 | 06:59:18.54 -21:11:00.4 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.8395-21.1845,2461098.6259,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.8395-21.1845 20260227.1259 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/CMa-03-Q1b1x1_2026-02-10_21-56-42_20.00sec_-15.00C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-03-Q1b1x1_210205_TTUQ1b1x1_14914_mhX3LLXV/fd_CMa-03-Q1b1x1_2026-02-26_21-00-44_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-03-Q1b1x1_210205_TTUQ1b1x1_14914_mhX3LLXV/fd_CMa-03-Q1b1x1_2026-02-26_21-01-25_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:18.54 -21:11:00.4 ;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_CMa-03-Q1b1x1_2026-02-10_21-56-42_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png resample_wcs_fd_CMa-03-Q1b1x1_2026-02-26_21-01-25_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-03-Q1b1x1_2026-02-10_21-56-42_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png resample_wcs_fd_CMa-03-Q1b1x1_2026-02-26_21-00-44_20_00sec_-14_90C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-03-Q1b1x1_2026-02-10_21-56-42_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png resample_wcs_fd_CMa-03-Q1b1x1_2026-02-26_21-01-25_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-03-Q1b1x1_2026-02-10_21-56-42_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png resample_wcs_fd_CMa-03-Q1b1x1_2026-02-26_21-00-44_20_00sec_-14_90C_LIGHT_0069_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1291* 03 10 53.52 +15 31 38.0 12.6 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6291,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1291 12.56CV 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:10:53.52 +15:31:38.0 ;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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1291* 02 48 42.09 +12 12 53.9 13.8 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6291,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1291 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:48:42.09 +12:12:53.9 ;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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1291* 02 51 40.70 +11 27 41.2 14.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6291,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1291 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:51:40.70 +11:27:41.2 ;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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1291* 02 33 57.56 +16 56 14.2 14.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6291,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1291 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:33:57.56 +16:56:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6311,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1311 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/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:28.19 +27:34:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1311* 01 51 51.14 +30 53 52.7 14.3 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6311,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1311 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/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:51.14 +30:53:52.7 ;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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1332 2461098.6332 12.63 20:15:53.29 +65:05:25.5
98.78323 16.17327 galactic Dra Second-epoch detections are separated by 0.8" 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 | Gaia DR3 2244815513966539008 | 20:15:52.71 +65:05:19.2 (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 2244815513966539008,2461098.6332,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2244815513966539008 20260227.1332 12.63CV 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/Cep-04-Q1b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-04-Q1b1x1_211235_TTUQ1b1x1_21193_0qpJ0pvj/fd_Cep-04-Q1b1x1_2026-02-26_21-11-18_20.00sec_-14.90C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-04-Q1b1x1_211235_TTUQ1b1x1_21193_0qpJ0pvj/fd_Cep-04-Q1b1x1_2026-02-26_21-11-55_20.00sec_-15.00C_LIGHT_0081.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:15:53.29 +65:05:25.5 ;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_Cep-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-02-26_21-11-55_20_00sec_-15_00C_LIGHT_0081_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-02-26_21-11-18_20_00sec_-14_90C_LIGHT_0080_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-02-26_21-11-55_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-02-26_21-11-18_20_00sec_-14_90C_LIGHT_0080_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1343* 03 25 14.70 -02 49 25.7 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6343,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1343 12.34CV 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/Eri-01-Q1b1x1_2025-12-22_23-08-35_20.00sec_-15.00C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Eri-01-Q1b1x1_211420_TTUQ1b1x1_16396_o4w65BEO/fd_Eri-01-Q1b1x1_2026-02-26_21-12-56_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Eri-01-Q1b1x1_211420_TTUQ1b1x1_16396_o4w65BEO/fd_Eri-01-Q1b1x1_2026-02-26_21-13-36_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:14.70 -02:49:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-01-Q1b1x1_2025-12-22_23-08-35_20_00sec_-15_00C_LIGHT_0220_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2026-02-26_21-13-36_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-01-Q1b1x1_2025-12-22_23-08-35_20_00sec_-15_00C_LIGHT_0220_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2026-02-26_21-12-56_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-22_23-08-35_20_00sec_-15_00C_LIGHT_0220_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2026-02-26_21-13-36_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-01-Q1b1x1_2025-12-22_23-08-35_20_00sec_-15_00C_LIGHT_0220_fits__*pix.png resample_wcs_fd_Eri-01-Q1b1x1_2026-02-26_21-12-56_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1363 2461098.6363 11.46 01:04:35.64 +41:17:56.1
125.58726 -21.50499 galactic And Second-epoch detections are separated by 0.5" and 8.2 pix This object is listed in neverexclude_list.txt 2.0" RX And - radio detected CVThe object was found in VSX 2" RX And
Type: UGZ
# Max. Min./Amp. JD0 Period
10.300 V 14.800 V 0.209893000000 pec(UG)
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1363* 01 04 35.64 +41 17 56.1 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RX And,2461098.6363,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX And 20260227.1363 11.46CV 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/And-02-Q1b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-02-Q1b1x1_211720_TTUQ1b1x1_2868_WGW9wA6r/fd_And-02-Q1b1x1_2026-02-26_21-15-32_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-02-Q1b1x1_211720_TTUQ1b1x1_2868_WGW9wA6r/fd_And-02-Q1b1x1_2026-02-26_21-16-33_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:04:35.64 +41:17:56.1 ;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_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-16-33_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-15-32_20_00sec_-15_00C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-16-33_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-15-32_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1363 2461098.6363 13.64 01:55:16.58 +47:56:49.0
133.85314 -13.56650 galactic Per Second-epoch detections are separated by 1.6" and 7.1 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 356344301156128000 | 01:55:18.29 +47:56:39.3 (Gaia DR3) | T | P | 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 02 27.1363* 01 55 16.58 +47 56 49.0 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 356344301156128000,2461098.6363,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 356344301156128000 20260227.1363 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/And-02-Q1b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-02-Q1b1x1_211720_TTUQ1b1x1_2868_WGW9wA6r/fd_And-02-Q1b1x1_2026-02-26_21-15-32_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-02-Q1b1x1_211720_TTUQ1b1x1_2868_WGW9wA6r/fd_And-02-Q1b1x1_2026-02-26_21-16-33_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:16.58 +47:56:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-16-33_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-15-32_20_00sec_-15_00C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-16-33_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-15-32_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1363 2461098.6363 11.44 01:04:35.63 +41:17:56.5
125.58722 -21.50488 galactic And Second-epoch detections are separated by 0.6" and 8.2 pix This object is listed in neverexclude_list.txt 1.6" RX And - radio detected CVThe object was found in VSX 2" RX And
Type: UGZ
# Max. Min./Amp. JD0 Period
10.300 V 14.800 V 0.209893000000 pec(UG)
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1363* 01 04 35.63 +41 17 56.5 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RX And,2461098.6363,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX And 20260227.1363 11.44CV 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/And-02-Q1b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q1b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-02-Q1b1x1_211720_TTUQ1b1x1_2868_WGW9wA6r/fd_And-02-Q1b1x1_2026-02-26_21-15-32_20.00sec_-15.00C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-02-Q1b1x1_211720_TTUQ1b1x1_2868_WGW9wA6r/fd_And-02-Q1b1x1_2026-02-26_21-16-33_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:04:35.63 +41:17:56.5 ;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_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-16-33_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-15-32_20_00sec_-15_00C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-16-33_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q1b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_fd_And-02-Q1b1x1_2026-02-26_21-15-32_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1392* 02 46 28.67 +23 21 36.5 13.0 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6392,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1392 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/Ari-03-Q1b1x1_2025-12-22_23-34-55_20.00sec_-15.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20.00sec_-14.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20.00sec_-15.00C_LIGHT_0091.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:46:28.67 +23:21:36.5 ;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_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1392* 03 16 06.72 +19 34 29.5 13.6 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6392,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1392 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/Ari-03-Q1b1x1_2025-12-22_23-34-55_20.00sec_-15.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20.00sec_-14.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20.00sec_-15.00C_LIGHT_0091.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:06.72 +19:34:29.5 ;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_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1392* 03 00 59.59 +25 59 12.3 14.2 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6392,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1392 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/Ari-03-Q1b1x1_2025-12-22_23-34-55_20.00sec_-15.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20.00sec_-14.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20.00sec_-15.00C_LIGHT_0091.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:59.59 +25:59:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1392* 02 53 27.76 +23 08 30.0 14.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6392,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1392 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/Ari-03-Q1b1x1_2025-12-22_23-34-55_20.00sec_-15.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20.00sec_-14.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20.00sec_-15.00C_LIGHT_0091.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:53:27.76 +23:08:30.0 ;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_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1392* 02 43 26.09 +18 34 12.8 14.5 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6392,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1392 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/Ari-03-Q1b1x1_2025-12-22_23-34-55_20.00sec_-15.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20.00sec_-14.90C_LIGHT_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-03-Q1b1x1_212135_TTUQ1b1x1_22985_eCrOcvGj/fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20.00sec_-15.00C_LIGHT_0091.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:43:26.09 +18:34:12.8 ;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_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-20-46_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-03-Q1b1x1_2025-12-22_23-34-55_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png resample_wcs_fd_Ari-03-Q1b1x1_2026-02-26_21-19-54_20_00sec_-14_90C_LIGHT_0090_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1412* 02 27 13.25 +40 06 56.5 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6412,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1412 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/And-06-Q1b1x1_2025-12-22_23-28-06_20.00sec_-15.00C_LIGHT_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-06-Q1b1x1_212420_TTUQ1b1x1_18549_NiASGfFH/fd_And-06-Q1b1x1_2026-02-26_21-22-42_20.00sec_-15.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-06-Q1b1x1_212420_TTUQ1b1x1_18549_NiASGfFH/fd_And-06-Q1b1x1_2026-02-26_21-23-40_20.00sec_-15.00C_LIGHT_0094.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:27:13.25 +40:06:56.5 ;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_And-06-Q1b1x1_2025-12-22_23-28-06_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png resample_wcs_fd_And-06-Q1b1x1_2026-02-26_21-23-40_20_00sec_-15_00C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-06-Q1b1x1_2025-12-22_23-28-06_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png resample_wcs_fd_And-06-Q1b1x1_2026-02-26_21-22-42_20_00sec_-15_00C_LIGHT_0093_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-06-Q1b1x1_2025-12-22_23-28-06_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png resample_wcs_fd_And-06-Q1b1x1_2026-02-26_21-23-40_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-06-Q1b1x1_2025-12-22_23-28-06_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png resample_wcs_fd_And-06-Q1b1x1_2026-02-26_21-22-42_20_00sec_-15_00C_LIGHT_0093_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1446* 05 34 15.77 -06 36 04.5 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
SW Ori,2461098.6446,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SW Ori 20260227.1446 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/Eri-05-Q1b1x1_2025-12-22_23-54-22_20.00sec_-14.90C_LIGHT_0272.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-05-Q1b1x1_2025-12-22_23-55-03_20.00sec_-15.00C_LIGHT_0273.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Eri-05-Q1b1x1_212905_TTUQ1b1x1_28239_5RznWK6w/fd_Eri-05-Q1b1x1_2026-02-26_21-27-47_20.00sec_-15.00C_LIGHT_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Eri-05-Q1b1x1_212905_TTUQ1b1x1_28239_5RznWK6w/fd_Eri-05-Q1b1x1_2026-02-26_21-28-24_20.00sec_-14.90C_LIGHT_0099.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:15.77 -06:36:04.5 ;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_Eri-05-Q1b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q1b1x1_2026-02-26_21-28-24_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-05-Q1b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q1b1x1_2026-02-26_21-27-47_20_00sec_-15_00C_LIGHT_0098_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-05-Q1b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q1b1x1_2026-02-26_21-28-24_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-05-Q1b1x1_2025-12-22_23-54-22_20_00sec_-14_90C_LIGHT_0272_fits__*pix.png resample_wcs_fd_Eri-05-Q1b1x1_2026-02-26_21-27-47_20_00sec_-15_00C_LIGHT_0098_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 39 17.63 +18 53 19.8 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6464,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1464 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:17.63 +18:53:19.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 35 07.00 +13 11 31.5 11.7 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
VARIABLE_NAME,2461098.6464,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1464 11.68CV 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/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:07.00 +13:11:31.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 10 54.87 +15 31 41.8 12.6 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6464,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1464 12.60CV 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/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:10:54.87 +15:31:41.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 25 36.35 +12 06 19.2 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,2461098.6464,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1464 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/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:36.35 +12:06:19.2 ;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_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 19 20.31 +18 24 59.6 13.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6464,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1464 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/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:20.31 +18:24:59.6 ;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_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 48 12.99 +14 28 39.9 13.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6464,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1464 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/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:12.99 +14:28:39.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 37 08.60 +12 15 31.4 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6464,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1464 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:08.60 +12:15:31.4 ;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_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 19 28.90 +17 04 45.8 14.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6464,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1464 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/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:28.90 +17:04:45.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1464* 03 57 54.70 +09 08 22.6 13.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1291 Tau,2461098.6464,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1291 Tau 20260227.1464 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/Tau-05-Q1b1x1_2025-12-22_23-48-17_20.00sec_-14.90C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2025-12-22_23-49-07_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-05-Q1b1x1_213150_TTUQ1b1x1_2458_IhR956gJ/fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20.00sec_-15.00C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:54.70 +09:08:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-31-06_20_00sec_-15_00C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-05-Q1b1x1_2025-12-22_23-48-17_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png resample_wcs_fd_Tau-05-Q1b1x1_2026-02-26_21-30-16_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1481* 04 23 45.63 +00 21 19.8 12.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6481,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1481 12.62CV 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/Eri-02-Q1b1x1_2025-12-22_23-45-40_20.00sec_-14.90C_LIGHT_0260.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Eri-02-Q1b1x1_213420_TTUQ1b1x1_3608_YAcO5ri3/fd_Eri-02-Q1b1x1_2026-02-26_21-32-44_20.00sec_-15.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Eri-02-Q1b1x1_213420_TTUQ1b1x1_3608_YAcO5ri3/fd_Eri-02-Q1b1x1_2026-02-26_21-33-32_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:45.63 +00:21:19.8 ;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_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-02-26_21-33-32_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-02-26_21-32-44_20_00sec_-15_00C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-02-26_21-33-32_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-02-26_21-32-44_20_00sec_-15_00C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1481 2461098.6481 12.68 04:39:30.08 -04:36:01.8
201.04115 -31.30060 galactic Eri Second-epoch detections are separated by 0.2" and 8.7 pix This object is listed in neverexclude_list.txt 3.5" BF Eri - AAVSO HST campaignThe object was found in VSX 3" BF Eri
Type: UG
# Max. Min./Amp. JD0 Period
12.300 V 15.200 V 0.270880400000 K3
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1481* 04 39 30.08 -04 36 01.8 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BF Eri,2461098.6481,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BF Eri 20260227.1481 12.68CV 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/Eri-02-Q1b1x1_2025-12-22_23-45-40_20.00sec_-14.90C_LIGHT_0260.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-02-Q1b1x1_2025-12-22_23-46-18_20.00sec_-14.90C_LIGHT_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Eri-02-Q1b1x1_213420_TTUQ1b1x1_3608_YAcO5ri3/fd_Eri-02-Q1b1x1_2026-02-26_21-32-44_20.00sec_-15.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Eri-02-Q1b1x1_213420_TTUQ1b1x1_3608_YAcO5ri3/fd_Eri-02-Q1b1x1_2026-02-26_21-33-32_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:30.08 -04:36:01.8 ;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_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-02-26_21-33-32_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-02-26_21-32-44_20_00sec_-15_00C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-02-26_21-33-32_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-02-26_21-32-44_20_00sec_-15_00C_LIGHT_0104_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1499* 03 01 00.68 +25 59 13.1 14.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6499,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1499 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/Ari-01-Q1b1x1_2025-12-22_23-51-31_20.00sec_-14.90C_LIGHT_0268.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-01-Q1b1x1_213650_TTUQ1b1x1_30528_mYCVSHti/fd_Ari-01-Q1b1x1_2026-02-26_21-35-20_20.00sec_-15.00C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-01-Q1b1x1_213650_TTUQ1b1x1_30528_mYCVSHti/fd_Ari-01-Q1b1x1_2026-02-26_21-36-01_20.00sec_-15.00C_LIGHT_0108.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:00.68 +25:59:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-26_21-36-01_20_00sec_-15_00C_LIGHT_0108_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-26_21-35-20_20_00sec_-15_00C_LIGHT_0107_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-26_21-36-01_20_00sec_-15_00C_LIGHT_0108_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-01-Q1b1x1_2025-12-22_23-51-31_20_00sec_-14_90C_LIGHT_0268_fits__*pix.png resample_wcs_fd_Ari-01-Q1b1x1_2026-02-26_21-35-20_20_00sec_-15_00C_LIGHT_0107_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1521* 03 59 07.66 +04 11 45.7 13.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6521,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1521 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-08-Q1b1x1_2025-12-23_00-04-48_20.00sec_-14.90C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20.00sec_-14.90C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20.00sec_-15.00C_LIGHT_0112.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:59:07.66 +04:11:45.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1521* 04 27 46.34 +10 04 35.3 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.6521,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1521 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/Tau-08-Q1b1x1_2025-12-23_00-04-48_20.00sec_-14.90C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20.00sec_-14.90C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20.00sec_-15.00C_LIGHT_0112.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:46.34 +10:04:35.3 ;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_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1521* 03 49 52.88 +01 10 17.9 14.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.6521,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1521 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/Tau-08-Q1b1x1_2025-12-23_00-04-48_20.00sec_-14.90C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20.00sec_-14.90C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20.00sec_-15.00C_LIGHT_0112.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:52.88 +01:10:17.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1521* 03 51 44.38 +08 22 03.7 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.6521,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1521 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/Tau-08-Q1b1x1_2025-12-23_00-04-48_20.00sec_-14.90C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20.00sec_-14.90C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20.00sec_-15.00C_LIGHT_0112.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:44.38 +08:22:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1521* 04 01 37.94 +07 25 40.9 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6521,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1521 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-08-Q1b1x1_2025-12-23_00-04-48_20.00sec_-14.90C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20.00sec_-14.90C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20.00sec_-15.00C_LIGHT_0112.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:37.94 +07:25:40.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1521* 04 16 10.21 +07 16 40.0 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,2461098.6521,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1521 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/Tau-08-Q1b1x1_2025-12-23_00-04-48_20.00sec_-14.90C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20.00sec_-14.90C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-08-Q1b1x1_213950_TTUQ1b1x1_16339_mJrBvYbH/fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20.00sec_-15.00C_LIGHT_0112.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:10.21 +07:16:40.0 ;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_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-39-04_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-08-Q1b1x1_2025-12-23_00-04-48_20_00sec_-14_90C_LIGHT_0284_fits__*pix.png resample_wcs_fd_Tau-08-Q1b1x1_2026-02-26_21-38-30_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1511 2461098.6511 14.04 02:18:16.63 +49:56:05.7
136.94796 -10.55878 galactic And Second-epoch detections are separated by 4.4" and 1.0 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 355568286465796480 | 02:18:18.49 +49:55:39.0 (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 02 27.1511* 02 18 16.63 +49 56 05.7 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 355568286465796480,2461098.6511,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 355568286465796480 20260227.1511 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/And-03-Q1b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-03-Q1b1x1_213820_TTUQ1b1x1_611_83T7Fmde/fd_And-03-Q1b1x1_2026-02-26_21-37-04_20.00sec_-15.00C_LIGHT_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-03-Q1b1x1_213820_TTUQ1b1x1_611_83T7Fmde/fd_And-03-Q1b1x1_2026-02-26_21-37-39_20.00sec_-14.90C_LIGHT_0110.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:18:16.63 +49:56:05.7 ;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_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-39_20_00sec_-14_90C_LIGHT_0110_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-04_20_00sec_-15_00C_LIGHT_0109_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-39_20_00sec_-14_90C_LIGHT_0110_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-04_20_00sec_-15_00C_LIGHT_0109_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1511* 03 01 22.19 +48 48 35.0 14.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.6511,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1511 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/And-03-Q1b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-03-Q1b1x1_213820_TTUQ1b1x1_611_83T7Fmde/fd_And-03-Q1b1x1_2026-02-26_21-37-04_20.00sec_-15.00C_LIGHT_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-03-Q1b1x1_213820_TTUQ1b1x1_611_83T7Fmde/fd_And-03-Q1b1x1_2026-02-26_21-37-39_20.00sec_-14.90C_LIGHT_0110.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:22.19 +48:48:35.0 ;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_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-39_20_00sec_-14_90C_LIGHT_0110_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-04_20_00sec_-15_00C_LIGHT_0109_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-39_20_00sec_-14_90C_LIGHT_0110_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-04_20_00sec_-15_00C_LIGHT_0109_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1511 2461098.6511 14.44 02:35:54.33 +41:23:20.2
143.17371 -17.34040 galactic And Second-epoch detections are separated by 7.9" and 0.8 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 J038.9839+41.3879 | 02:35:54.33 +41:23:20.2 (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 02 27.1511* 02 35 54.33 +41 23 20.2 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.9839+41.3879,2461098.6511,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.9839+41.3879 20260227.1511 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/And-03-Q1b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-03-Q1b1x1_213820_TTUQ1b1x1_611_83T7Fmde/fd_And-03-Q1b1x1_2026-02-26_21-37-04_20.00sec_-15.00C_LIGHT_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-03-Q1b1x1_213820_TTUQ1b1x1_611_83T7Fmde/fd_And-03-Q1b1x1_2026-02-26_21-37-39_20.00sec_-14.90C_LIGHT_0110.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:35:54.33 +41:23:20.2 ;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_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-39_20_00sec_-14_90C_LIGHT_0110_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-04_20_00sec_-15_00C_LIGHT_0109_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-39_20_00sec_-14_90C_LIGHT_0110_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-04_20_00sec_-15_00C_LIGHT_0109_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1511* 01 58 38.84 +44 10 36.3 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6511,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1511 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/And-03-Q1b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-03-Q1b1x1_213820_TTUQ1b1x1_611_83T7Fmde/fd_And-03-Q1b1x1_2026-02-26_21-37-04_20.00sec_-15.00C_LIGHT_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_And-03-Q1b1x1_213820_TTUQ1b1x1_611_83T7Fmde/fd_And-03-Q1b1x1_2026-02-26_21-37-39_20.00sec_-14.90C_LIGHT_0110.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:58:38.84 +44:10:36.3 ;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_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-39_20_00sec_-14_90C_LIGHT_0110_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-04_20_00sec_-15_00C_LIGHT_0109_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-39_20_00sec_-14_90C_LIGHT_0110_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-02-26_21-37-04_20_00sec_-15_00C_LIGHT_0109_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1539* 03 40 21.90 +19 23 07.6 7.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6539,7.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1539 7.57CV 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/Tau-02-Q1b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:21.90 +19:23:07.6 ;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_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1539* 03 39 18.23 +18 53 23.5 11.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6539,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1539 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q1b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:18.23 +18:53:23.5 ;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_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1539* 03 40 21.89 +19 23 07.5 8.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6539,7.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1539 7.96CV 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/Tau-02-Q1b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:21.89 +19:23:07.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1539* 03 46 43.90 +24 57 08.9 12.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6539,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1539 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q1b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:43.90 +24:57:08.9 ;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_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1539* 03 33 37.74 +20 43 51.0 12.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6539,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1539 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q1b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:33:37.74 +20:43:51.0 ;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_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1539* 03 19 20.72 +18 25 01.6 13.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6539,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1539 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q1b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:20.72 +18:25:01.6 ;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_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1539* 03 16 07.80 +19 34 32.8 13.5 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6539,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1539 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/Tau-02-Q1b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:07.80 +19:34:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1539* 03 40 07.78 +26 07 00.7 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6539,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1539 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q1b1x1_2025-12-23_00-08-13_20.00sec_-15.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tau-02-Q1b1x1_214235_TTUQ1b1x1_22213_unPnFER8/fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20.00sec_-15.00C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:07.78 +26:07:00.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-41-52_20_00sec_-15_00C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q1b1x1_2025-12-23_00-08-13_20_00sec_-15_00C_LIGHT_0288_fits__*pix.png resample_wcs_fd_Tau-02-Q1b1x1_2026-02-26_21-40-56_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1559 2461098.6559 11.89 06:40:29.27 -21:35:51.2
231.24269 -11.96785 galactic CMa Second-epoch detections are separated by 5.6" and 7.3 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 2926675794508587648 | 06:40:30.41 -21:35:46.5 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2926675794508587648,2461098.6559,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2926675794508587648 20260227.1559 11.89CV 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/CMa-01-Q1b1x1_2025-12-22_23-57-47_20.00sec_-15.00C_LIGHT_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-01-Q1b1x1_214535_TTUQ1b1x1_13800_PRkyeNk9/fd_CMa-01-Q1b1x1_2026-02-26_21-43-40_20.00sec_-14.90C_LIGHT_0117.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-01-Q1b1x1_214535_TTUQ1b1x1_13800_PRkyeNk9/fd_CMa-01-Q1b1x1_2026-02-26_21-44-54_20.00sec_-14.90C_LIGHT_0118.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:29.27 -21:35:51.2 ;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_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-02-26_21-44-54_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-02-26_21-43-40_20_00sec_-14_90C_LIGHT_0117_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-02-26_21-44-54_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-02-26_21-43-40_20_00sec_-14_90C_LIGHT_0117_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1559 2461098.6559 12.75 05:44:05.15 -21:29:55.3
225.78967 -24.01482 galactic Lep Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:44:05.15 -21:29:55.3 (user input) | T | P | (position from user input) J-Ks=0.302+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.6559,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1559 12.75CV 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/CMa-01-Q1b1x1_2025-12-22_23-57-47_20.00sec_-15.00C_LIGHT_0276.fits /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q1b1x1_2025-12-22_23-58-36_20.00sec_-15.00C_LIGHT_0277.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-01-Q1b1x1_214535_TTUQ1b1x1_13800_PRkyeNk9/fd_CMa-01-Q1b1x1_2026-02-26_21-43-40_20.00sec_-14.90C_LIGHT_0117.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_CMa-01-Q1b1x1_214535_TTUQ1b1x1_13800_PRkyeNk9/fd_CMa-01-Q1b1x1_2026-02-26_21-44-54_20.00sec_-14.90C_LIGHT_0118.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:05.15 -21:29:55.3 ;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_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-02-26_21-44-54_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-02-26_21-43-40_20_00sec_-14_90C_LIGHT_0117_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-02-26_21-44-54_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-02-26_21-43-40_20_00sec_-14_90C_LIGHT_0117_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1581* 03 30 03.07 +35 40 16.1 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
R Per,2461098.6581,8.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
R Per 20260227.1581 8.63CV 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/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-04-Q1b1x1_214835_TTUQ1b1x1_30164_HYwiXZsT/fd_Per-04-Q1b1x1_2026-02-26_21-47-16_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-04-Q1b1x1_214835_TTUQ1b1x1_30164_HYwiXZsT/fd_Per-04-Q1b1x1_2026-02-26_21-47-51_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:30:03.07 +35:40:16.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-26_21-47-51_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-26_21-47-16_20_00sec_-14_90C_LIGHT_0120_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-26_21-47-51_20_00sec_-15_00C_LIGHT_0121_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-26_21-47-16_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1581* 03 39 28.78 +33 03 07.1 13.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6581,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1581 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/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-04-Q1b1x1_214835_TTUQ1b1x1_30164_HYwiXZsT/fd_Per-04-Q1b1x1_2026-02-26_21-47-16_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Per-04-Q1b1x1_214835_TTUQ1b1x1_30164_HYwiXZsT/fd_Per-04-Q1b1x1_2026-02-26_21-47-51_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:28.78 +33:03:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-26_21-47-51_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-26_21-47-16_20_00sec_-14_90C_LIGHT_0120_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-26_21-47-51_20_00sec_-15_00C_LIGHT_0121_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-26_21-47-16_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1602 2461098.6602 12.45 09:32:40.78 -32:03:03.2
261.11017 14.24224 galactic Ant Second-epoch detections are separated by 0.7" and 6.7 pix
The object was found in VSX 1" ASASSN-V J093240.85-320302.7
Type: SR
# Max. Min./Amp. JD0 Period
13.060 V 14.100 V 2457874.60000 239.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1602* 09 32 40.78 -32 03 03.2 12.4 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J093240.85-320302.7,2461098.6602,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J093240.85-320302.7 20260227.1602 12.45CV 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/Pyx-02-Q1b1x1_2026-01-09_02-33-25_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-02-Q1b1x1_2026-01-09_02-34-15_20.00sec_-15.00C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pyx-02-Q1b1x1_215150_TTUQ1b1x1_8587_ByV8Nyhm/fd_Pyx-02-Q1b1x1_2026-02-26_21-50-00_20.00sec_-14.90C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Pyx-02-Q1b1x1_215150_TTUQ1b1x1_8587_ByV8Nyhm/fd_Pyx-02-Q1b1x1_2026-02-26_21-51-08_20.00sec_-15.00C_LIGHT_0124.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:32:40.78 -32:03:03.2 ;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_Pyx-02-Q1b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q1b1x1_2026-02-26_21-51-08_20_00sec_-15_00C_LIGHT_0124_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-02-Q1b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q1b1x1_2026-02-26_21-50-00_20_00sec_-14_90C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q1b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q1b1x1_2026-02-26_21-51-08_20_00sec_-15_00C_LIGHT_0124_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-02-Q1b1x1_2026-01-09_02-33-25_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Pyx-02-Q1b1x1_2026-02-26_21-50-00_20_00sec_-14_90C_LIGHT_0123_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1627 2461098.6627 12.13 11:04:29.98 -30:02:05.7
276.91850 27.37963 galactic Hya Second-epoch detections are separated by 0.4" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5452541594513191680 | 11:04:30.04 -30:02:05.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.545+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 5452541594513191680,2461098.6627,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5452541594513191680 20260227.1627 12.13CV 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/Hya-10-Q1b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q1b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q1b1x1_215638_TTUQ1b1x1_30793_gBXvkUKz/fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20.00sec_-14.90C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q1b1x1_215638_TTUQ1b1x1_30793_gBXvkUKz/fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20.00sec_-15.00C_LIGHT_0128.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:04:29.98 -30:02:05.7 ;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_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20_00sec_-15_00C_LIGHT_0128_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20_00sec_-14_90C_LIGHT_0127_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20_00sec_-15_00C_LIGHT_0128_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20_00sec_-14_90C_LIGHT_0127_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 5453228991144244096,2461098.6627,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5453228991144244096 20260227.1627 12.64CV 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/Hya-10-Q1b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q1b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q1b1x1_215638_TTUQ1b1x1_30793_gBXvkUKz/fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20.00sec_-14.90C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q1b1x1_215638_TTUQ1b1x1_30793_gBXvkUKz/fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20.00sec_-15.00C_LIGHT_0128.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:57:14.11 -29:28:26.0 ;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_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20_00sec_-15_00C_LIGHT_0128_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20_00sec_-14_90C_LIGHT_0127_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20_00sec_-15_00C_LIGHT_0128_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20_00sec_-14_90C_LIGHT_0127_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1627 2461098.6627 12.45 10:58:31.74 -29:34:36.5
275.38791 27.18737 galactic Hya Second-epoch detections are separated by 1.3" and 1.8 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 J164.6296-29.5691 | 10:58:31.79 -29:34:36.9 (Gaia DR3) | CBF (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.215+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J164.6296-29.5691,2461098.6627,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164.6296-29.5691 20260227.1627 12.45CV 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/Hya-10-Q1b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q1b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q1b1x1_215638_TTUQ1b1x1_30793_gBXvkUKz/fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20.00sec_-14.90C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q1b1x1_215638_TTUQ1b1x1_30793_gBXvkUKz/fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20.00sec_-15.00C_LIGHT_0128.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:58:31.74 -29:34:36.5 ;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_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20_00sec_-15_00C_LIGHT_0128_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20_00sec_-14_90C_LIGHT_0127_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-54-27_20_00sec_-15_00C_LIGHT_0128_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-10-Q1b1x1_2026-01-21_02-59-12_20_00sec_-15_00C_LIGHT_0426_fits__*pix.png resample_wcs_fd_Hya-10-Q1b1x1_2026-02-26_21-53-50_20_00sec_-14_90C_LIGHT_0127_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6680,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1680 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q1b1x1_220354_TTUQ1b1x1_9915_eXqvZwBM/fd_Hya-09-Q1b1x1_2026-02-26_22-01-24_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q1b1x1_220354_TTUQ1b1x1_9915_eXqvZwBM/fd_Hya-09-Q1b1x1_2026-02-26_22-02-06_20.00sec_-15.00C_LIGHT_0138.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:11:13.22 -18:57:25.3 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-26_22-02-06_20_00sec_-15_00C_LIGHT_0138_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-26_22-01-24_20_00sec_-14_90C_LIGHT_0137_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-26_22-02-06_20_00sec_-15_00C_LIGHT_0138_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-26_22-01-24_20_00sec_-14_90C_LIGHT_0137_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6670,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1670 13.18CV 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/Hya-06-Q1b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-06-Q1b1x1_220531_TTUQ1b1x1_17645_23dGHO5Q/fd_Hya-06-Q1b1x1_2026-02-26_21-59-56_20.00sec_-14.90C_LIGHT_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-06-Q1b1x1_220531_TTUQ1b1x1_17645_23dGHO5Q/fd_Hya-06-Q1b1x1_2026-02-26_22-00-37_20.00sec_-15.00C_LIGHT_0136.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:08.18 -08:31:40.9 ;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_Hya-06-Q1b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q1b1x1_2026-02-26_22-00-37_20_00sec_-15_00C_LIGHT_0136_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q1b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q1b1x1_2026-02-26_21-59-56_20_00sec_-14_90C_LIGHT_0135_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q1b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q1b1x1_2026-02-26_22-00-37_20_00sec_-15_00C_LIGHT_0136_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q1b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q1b1x1_2026-02-26_21-59-56_20_00sec_-14_90C_LIGHT_0135_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1723* 11 19 27.32 -06 17 09.2 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6723,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1723 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/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-01-Q1b1x1_220951_TTUQ1b1x1_10788_eC8ikLZc/fd_Crt-01-Q1b1x1_2026-02-26_22-07-36_20.00sec_-15.00C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-01-Q1b1x1_220951_TTUQ1b1x1_10788_eC8ikLZc/fd_Crt-01-Q1b1x1_2026-02-26_22-08-22_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:19:27.32 -06:17:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q1b1x1_2026-02-26_22-08-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q1b1x1_2026-02-26_22-07-36_20_00sec_-15_00C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q1b1x1_2026-02-26_22-08-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q1b1x1_2026-02-26_22-07-36_20_00sec_-15_00C_LIGHT_0144_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6704,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1704 10.68CV 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/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q1b1x1_221347_TTUQ1b1x1_901_tXBtymr2/fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20.00sec_-14.90C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q1b1x1_221347_TTUQ1b1x1_901_tXBtymr2/fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20.00sec_-14.90C_LIGHT_0142.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:42.17 +02:27:25.2 ;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_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20_00sec_-14_90C_LIGHT_0142_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20_00sec_-14_90C_LIGHT_0141_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20_00sec_-14_90C_LIGHT_0142_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20_00sec_-14_90C_LIGHT_0141_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1704* 09 54 11.66 +02 00 15.6 13.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6704,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1704 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/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q1b1x1_221347_TTUQ1b1x1_901_tXBtymr2/fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20.00sec_-14.90C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q1b1x1_221347_TTUQ1b1x1_901_tXBtymr2/fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20.00sec_-14.90C_LIGHT_0142.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:54:11.66 +02:00:15.6 ;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_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20_00sec_-14_90C_LIGHT_0142_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20_00sec_-14_90C_LIGHT_0141_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20_00sec_-14_90C_LIGHT_0142_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20_00sec_-14_90C_LIGHT_0141_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1704* 09 44 17.18 +02 09 04.9 13.8 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6704,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1704 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/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q1b1x1_221347_TTUQ1b1x1_901_tXBtymr2/fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20.00sec_-14.90C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q1b1x1_221347_TTUQ1b1x1_901_tXBtymr2/fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20.00sec_-14.90C_LIGHT_0142.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:44:17.18 +02:09:04.9 ;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_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20_00sec_-14_90C_LIGHT_0142_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20_00sec_-14_90C_LIGHT_0141_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20_00sec_-14_90C_LIGHT_0142_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20_00sec_-14_90C_LIGHT_0141_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6704,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1704 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/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q1b1x1_221347_TTUQ1b1x1_901_tXBtymr2/fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20.00sec_-14.90C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-04-Q1b1x1_221347_TTUQ1b1x1_901_tXBtymr2/fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20.00sec_-14.90C_LIGHT_0142.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:14:51.93 +03:04:00.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20_00sec_-14_90C_LIGHT_0142_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20_00sec_-14_90C_LIGHT_0141_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-05-36_20_00sec_-14_90C_LIGHT_0142_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-26_22-04-40_20_00sec_-14_90C_LIGHT_0141_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 10.76 12:05:15.72 -20:29:57.7
288.53343 41.07780 galactic Crv Second-epoch detections are separated by 2.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3518457004388520064 | 12:05:15.63 -20:29:56.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.793+/-0.038 (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
Gaia DR3 3518457004388520064,2461098.6733,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3518457004388520064 20260227.1733 10.76CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:05:15.72 -20:29:57.7 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
W Crt,2461098.6733,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
W Crt 20260227.1733 10.83CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:26:29.61 -17:54:51.5 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 9.73 12:05:28.33 -22:26:05.6
289.18440 39.20668 galactic Crv Second-epoch detections are separated by 1.5" 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 | Gaia DR3 3493217818052242688 | 12:05:27.90 -22:25:59.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5V 1980AJ.....85.1366S HD 105023
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 3493217818052242688,2461098.6733,9.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493217818052242688 20260227.1733 9.73CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:05:28.33 -22:26:05.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 10.16 12:06:18.17 -22:17:32.5
289.38427 39.38910 galactic Crv Second-epoch detections are separated by 1.5" 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 3493225892590772608 | 12:06:17.88 -22:17:27.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3493225892590772608,2461098.6733,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493225892590772608 20260227.1733 10.16CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:06:18.17 -22:17:32.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 10.53 12:06:04.85 -22:51:14.1
289.48273 38.83041 galactic Crv Second-epoch detections are separated by 3.2" 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 3493133671053025792 | 12:06:04.51 -22:51:08.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3493133671053025792,2461098.6733,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493133671053025792 20260227.1733 10.53CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:06:04.85 -22:51:14.1 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 11.89 12:05:48.63 -22:45:33.5
289.37738 38.90854 galactic Crv Second-epoch detections are separated by 6.6" 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 3493138103459277824 | 12:05:48.07 -22:45:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3493138103459277824,2461098.6733,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493138103459277824 20260227.1733 11.89CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:05:48.63 -22:45:33.5 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.14 12:05:26.78 -22:43:08.8
289.26055 38.92861 galactic Crv Second-epoch detections are separated by 6.0" 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 3493139061235779072 | 12:05:26.20 -22:43:01.2 (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 3493139061235779072,2461098.6733,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493139061235779072 20260227.1733 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:05:26.78 -22:43:08.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.42 12:05:49.09 -22:25:54.8
289.28400 39.22783 galactic Crv Second-epoch detections are separated by 1.3" 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 | Gaia DR3 3493217268296432128 | 12:05:48.79 -22:25:50.4 (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 3493217268296432128,2461098.6733,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493217268296432128 20260227.1733 12.42CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:05:49.09 -22:25:54.8 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.49 12:05:20.44 -22:45:12.3
289.24013 38.88965 galactic Crv Second-epoch detections are separated by 5.8" 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 3493138889437088768 | 12:05:19.84 -22:45:04.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3493138889437088768,2461098.6733,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493138889437088768 20260227.1733 12.49CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:05:20.44 -22:45:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.60 11:58:23.97 -21:54:02.2
286.96461 39.32102 galactic Crv Second-epoch detections are separated by 7.2" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3493874673171272064 | 11:58:24.15 -21:53:56.2 (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 3493874673171272064,2461098.6733,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493874673171272064 20260227.1733 12.60CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:58:23.97 -21:54:02.2 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.63 12:06:08.32 -22:31:44.5
289.40541 39.14997 galactic Crv Second-epoch detections are separated by 2.7" 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 | Gaia DR3 3493212835890243072 | 12:06:07.94 -22:31:39.4 (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 3493212835890243072,2461098.6733,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493212835890243072 20260227.1733 12.63CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:06:08.32 -22:31:44.5 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.73 12:06:14.84 -22:34:12.2
289.44882 39.11564 galactic Crv Second-epoch detections are separated by 4.0" 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 | Gaia DR3 3493165556890246528 | 12:06:14.51 -22:34:07.3 (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 3493165556890246528,2461098.6733,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493165556890246528 20260227.1733 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:06:14.84 -22:34:12.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6733,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1733 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:03:20.04 -22:43:48.1 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
SN 1974E,2461098.6733,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SN 1974E 20260227.1733 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:01:53.54 -18:52:00.5 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.87 12:05:30.67 -22:48:31.2
289.30545 38.84481 galactic Crv Second-epoch detections are separated by 5.0" 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 3493136248033402624 | 12:05:30.07 -22:48:23.6 (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 3493136248033402624,2461098.6733,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493136248033402624 20260227.1733 12.87CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:05:30.67 -22:48:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.29 12:00:11.30 -19:05:40.7
286.51644 42.13769 galactic Crv Second-epoch detections are separated by 1.8" 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 3566877877272728448 | 12:00:11.37 -19:05:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.615+/-0.032 (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
Gaia DR3 3566877877272728448,2461098.6733,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3566877877272728448 20260227.1733 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:00:11.30 -19:05:40.7 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 3494273417935271168,2461098.6733,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3494273417935271168 20260227.1733 11.94CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:01:22.16 -21:27:38.0 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 9.64 11:55:07.36 -22:17:16.6
286.15893 38.74265 galactic Crt 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 3493788808184663680 | 11:55:07.33 -22:17:15.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F1 1980AJ.....85.1366S HD 103523 J-Ks=0.199+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3493788808184663680,2461098.6733,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493788808184663680 20260227.1733 9.64CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:55:07.36 -22:17:16.6 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.02 11:59:44.45 -22:01:18.2
287.39341 39.28511 galactic Crv Second-epoch detections are separated by 0.9" 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 3493855259919166464 | 11:59:44.40 -22:01:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.030 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3493855259919166464,2461098.6733,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493855259919166464 20260227.1733 12.02CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:59:44.45 -22:01:18.2 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 12.34 11:56:53.28 -21:39:28.1
286.44300 39.46097 galactic Crv Second-epoch detections are separated by 2.9" 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 3493935352469172864 | 11:56:53.22 -21:39:28.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-0.036 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3493935352469172864,2461098.6733,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3493935352469172864 20260227.1733 12.34CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:56:53.28 -21:39:28.1 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 10.95 11:49:15.36 -22:19:58.9
284.51627 38.30492 galactic Crt 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 3492520487163017472 | 11:49:15.38 -22:19:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.032 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3492520487163017472,2461098.6733,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3492520487163017472 20260227.1733 10.95CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:49:15.36 -22:19:58.9 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1733 2461098.6733 10.37 11:59:44.59 -21:28:24.4
287.21053 39.81494 galactic Crv Second-epoch detections are separated by 0.3" 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 3494264724919722496 | 11:59:44.59 -21:28:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.726+/-0.037 (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
Gaia DR3 3494264724919722496,2461098.6733,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3494264724919722496 20260227.1733 10.37CV 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/Crt-02-Q1b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q1b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crt-02-Q1b1x1_221149_TTUQ1b1x1_32153_xXF0k0Pm/fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:59:44.59 -21:28:24.4 ;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_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-44_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q1b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q1b1x1_2026-02-26_22-09-08_20_00sec_-15_00C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1746* 10 28 40.41 +00 06 21.9 8.8 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6746,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1746 8.79CV 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20.00sec_-14.90C_LIGHT_0149.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:28:40.41 -00:06:21.9 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1746* 10 37 11.50 -01 35 42.8 12.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6746,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1746 12.45CV 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20.00sec_-14.90C_LIGHT_0149.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:37:11.50 -01:35:42.8 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1746* 09 54 11.45 +02 00 16.9 13.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6746,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1746 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20.00sec_-14.90C_LIGHT_0149.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:54:11.45 +02:00:16.9 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1746* 10 27 05.86 +00 42 26.7 13.9 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6746,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1746 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20.00sec_-14.90C_LIGHT_0149.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:27:05.86 +00:42:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1746* 10 41 05.31 -01 50 28.0 14.3 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6746,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1746 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20.00sec_-14.90C_LIGHT_0149.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:41:05.31 -01:50:28.0 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1746* 10 08 07.51 -04 37 11.6 14.3 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6746,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1746 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20.00sec_-14.90C_LIGHT_0149.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:08:07.51 -04:37:11.6 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1746* 10 00 11.31 +00 00 26.4 14.5 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6746,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1746 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20.00sec_-14.90C_LIGHT_0149.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:00:11.31 +00:00:26.4 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1746* 10 20 31.20 -01 50 40.8 13.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6746,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1746 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/Sex-02-Q1b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q1b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-02-Q1b1x1_221557_TTUQ1b1x1_29183_e1EwxTVF/fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20.00sec_-14.90C_LIGHT_0149.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:20:31.20 -01:50:40.8 ;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_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-11-48_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q1b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q1b1x1_2026-02-26_22-10-48_20_00sec_-15_00C_LIGHT_0148_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1777* 10 32 04.12 +05 31 41.3 11.6 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6777,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1777 11.60CV 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:32:04.12 +05:31:41.3 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1777* 09 53 28.59 +05 15 55.2 12.3 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6777,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1777 12.27CV 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:53:28.59 +05:15:55.2 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1777* 10 27 39.77 +06 16 54.5 13.2 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6777,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1777 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:27:39.77 +06:16:54.5 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1777* 09 54 11.27 +02 00 17.2 13.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6777,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1777 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:54:11.27 +02:00:17.2 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1777* 10 01 40.04 +03 46 34.8 14.1 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6777,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1777 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:01:40.04 +03:46:34.8 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1777* 10 35 35.89 +06 06 25.4 14.3 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6777,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1777 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:35:35.89 +06:06:25.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1805* 11 03 40.04 -01 38 34.1 11.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6805,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1805 11.51CV 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/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20.00sec_-15.00C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:40.04 -01:38:34.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1805* 11 11 21.95 -05 53 31.6 11.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TV Leo,2461098.6805,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TV Leo 20260227.1805 11.69CV 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/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20.00sec_-15.00C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:11:21.95 -05:53:31.6 ;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_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1805* 11 30 15.52 +00 57 58.4 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6805,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1805 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20.00sec_-15.00C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:30:15.52 -00:57:58.4 ;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_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1805* 11 36 40.87 -02 36 29.0 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6805,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1805 12.71CV 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/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20.00sec_-15.00C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:40.87 -02:36:29.0 ;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_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1805* 11 06 54.18 +00 52 56.1 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6805,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1805 12.84CV 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/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20.00sec_-15.00C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:06:54.18 -00:52:56.1 ;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_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1805 2461098.6805 12.94 11:21:26.08 -03:14:54.4
263.88406 52.66254 galactic Leo Second-epoch detections are separated by 1.1" and 9.4 pix This object is listed in comets.txt 4.7" 17.3mag 29P/Schwassmann-Wachmann 1
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.4.7" 17.3mag 29P/Schwassmann-Wachmann 1
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1805* 11 21 26.08 -03 14 54.4 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6805,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1805 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20.00sec_-15.00C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:21:26.08 -03:14:54.4 ;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_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1805* 11 05 59.36 -04 09 35.3 13.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6805,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1805 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/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20.00sec_-15.00C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:59.36 -04:09:35.3 ;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_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1805* 11 19 26.88 -06 17 09.2 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6805,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1805 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/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-08-Q1b1x1_222129_TTUQ1b1x1_20593_TvTmf7fm/fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20.00sec_-15.00C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:19:26.88 -06:17:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-20-09_20_00sec_-15_00C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q1b1x1_2026-02-26_22-19-22_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6794,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1794 13.16CV 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/Vir-10-Q1b1x1_2026-01-18_04-06-05_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Vir-10-Q1b1x1_222336_TTUQ1b1x1_15170_DyfxzrpZ/fd_Vir-10-Q1b1x1_2026-02-26_22-17-50_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Vir-10-Q1b1x1_222336_TTUQ1b1x1_15170_DyfxzrpZ/fd_Vir-10-Q1b1x1_2026-02-26_22-18-35_20.00sec_-15.00C_LIGHT_0156.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:12:22.18 -13:53:41.8 ;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_Vir-10-Q1b1x1_2026-01-18_04-06-05_20_00sec_-14_90C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Vir-10-Q1b1x1_2026-02-26_22-18-35_20_00sec_-15_00C_LIGHT_0156_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q1b1x1_2026-01-18_04-06-05_20_00sec_-14_90C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Vir-10-Q1b1x1_2026-02-26_22-17-50_20_00sec_-14_90C_LIGHT_0155_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q1b1x1_2026-01-18_04-06-05_20_00sec_-14_90C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Vir-10-Q1b1x1_2026-02-26_22-18-35_20_00sec_-15_00C_LIGHT_0156_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q1b1x1_2026-01-18_04-06-05_20_00sec_-14_90C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Vir-10-Q1b1x1_2026-02-26_22-17-50_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1794 2461098.6794 10.54 12:30:48.26 -14:30:47.2
295.44915 48.05863 galactic Crv Second-epoch detections are separated by 1.9" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3527620128135889024 | 12:30:48.28 -14:30:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.731+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3527620128135889024,2461098.6794,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3527620128135889024 20260227.1794 10.54CV 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/Vir-10-Q1b1x1_2026-01-18_04-06-05_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q1b1x1_2026-01-18_04-06-49_20.00sec_-15.00C_LIGHT_0480.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Vir-10-Q1b1x1_222336_TTUQ1b1x1_15170_DyfxzrpZ/fd_Vir-10-Q1b1x1_2026-02-26_22-17-50_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Vir-10-Q1b1x1_222336_TTUQ1b1x1_15170_DyfxzrpZ/fd_Vir-10-Q1b1x1_2026-02-26_22-18-35_20.00sec_-15.00C_LIGHT_0156.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:30:48.26 -14:30:47.2 ;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_Vir-10-Q1b1x1_2026-01-18_04-06-05_20_00sec_-14_90C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Vir-10-Q1b1x1_2026-02-26_22-18-35_20_00sec_-15_00C_LIGHT_0156_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q1b1x1_2026-01-18_04-06-05_20_00sec_-14_90C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Vir-10-Q1b1x1_2026-02-26_22-17-50_20_00sec_-14_90C_LIGHT_0155_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q1b1x1_2026-01-18_04-06-05_20_00sec_-14_90C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Vir-10-Q1b1x1_2026-02-26_22-18-35_20_00sec_-15_00C_LIGHT_0156_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q1b1x1_2026-01-18_04-06-05_20_00sec_-14_90C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Vir-10-Q1b1x1_2026-02-26_22-17-50_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1763 2461098.6763 12.44 03:58:18.99 +68:28:24.8
138.75415 11.55428 galactic Cam Second-epoch detections are separated by 6.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493779608198576640 | 03:58:15.05 +68:28:25.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493779608198576640,2461098.6763,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493779608198576640 20260227.1763 12.44CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20.00sec_-15.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20.00sec_-15.00C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:18.99 +68:28:24.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1763 2461098.6763 12.35 03:54:15.60 +74:39:39.0
134.29080 15.98157 galactic Cam Second-epoch detections are separated by 2.0" and 6.9 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 | 03:54:15.60 +74:39:39.0 (user input) | T | P | (position from user input) J-Ks=0.673+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6763,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1763 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20.00sec_-15.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20.00sec_-15.00C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:15.60 +74:39:39.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 493778100669253888,2461098.6763,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493778100669253888 20260227.1763 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20.00sec_-15.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20.00sec_-15.00C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:25.67 +68:22:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1763 2461098.6763 12.48 04:12:33.46 +69:52:50.2
138.71735 13.44586 galactic Cam Second-epoch detections are separated by 8.1" and 7.2 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 J063.1410+69.8818 | 04:12:33.46 +69:52:50.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J063.1410+69.8818,2461098.6763,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J063.1410+69.8818 20260227.1763 12.48CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20.00sec_-15.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20.00sec_-15.00C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:33.46 +69:52:50.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1763* 03 36 20.69 +73 19 22.2 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6763,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1763 12.40CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20.00sec_-15.00C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-06-Q1b1x1_221749_TTUQ1b1x1_15379_sGd5abci/fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20.00sec_-15.00C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:20.69 +73:19:22.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-14-17_20_00sec_-15_00C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-26_22-13-08_20_00sec_-15_00C_LIGHT_0150_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 38 24.84 +19 08 42.2 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 12.63CV 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:38:24.84 +19:08:42.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 40 31.85 +21 28 38.0 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:40:31.85 +21:28:38.0 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 01 30.35 +23 42 45.6 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:01:30.35 +23:42:45.6 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 09 37 07.46 +24 36 05.4 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:37:07.46 +24:36:05.4 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.1817 2461098.6817 13.77 09:38:32.36 +19:24:48.5
212.17384 45.29768 galactic Leo Second-epoch detections are separated by 5.0" and 3.8 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 633645875323090944 | 09:38:35.59 +19:24:46.4 (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 02 27.1817* 09 38 32.36 +19 24 48.5 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 633645875323090944,2461098.6817,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 633645875323090944 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:38:32.36 +19:24:48.5 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 08 50.60 +19 32 36.3 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:08:50.60 +19:32:36.3 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 09 42.63 +18 45 23.2 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,14.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:42.63 +18:45:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 00 02.39 +22 37 52.8 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:00:02.39 +22:37:52.8 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 10 16 25.62 +17 41 46.1 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:16:25.62 +17:41:46.1 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1817* 09 58 05.41 +21 46 54.1 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6817,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1817 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/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-02-Q1b1x1_222536_TTUQ1b1x1_29841_s8xD0Ccz/fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20.00sec_-15.00C_LIGHT_0160.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:58:05.41 +21:46:54.1 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-49_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-26_22-21-12_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1847* 10 50 19.20 +10 44 32.3 11.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6846,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1846 11.46CV 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/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20.00sec_-14.90C_LIGHT_0165.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:50:19.20 +10:44:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1847* 11 12 43.44 +07 56 16.8 11.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6846,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1846 11.68CV 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/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20.00sec_-14.90C_LIGHT_0165.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:12:43.44 +07:56:16.8 ;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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1847* 11 36 57.77 +06 54 10.9 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6846,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1846 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20.00sec_-14.90C_LIGHT_0165.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:57.77 +06:54:10.9 ;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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1847* 11 36 15.87 +05 49 52.0 13.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6846,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1846 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/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20.00sec_-14.90C_LIGHT_0165.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:36:15.87 +05:49:52.0 ;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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1847* 11 37 37.76 +07 33 32.4 13.8 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6846,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1846 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/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-07-Q1b1x1_222931_TTUQ1b1x1_25542_BnYrSQbF/fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20.00sec_-14.90C_LIGHT_0165.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:37.76 +07:33:32.4 ;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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-26-10_20_00sec_-14_90C_LIGHT_0165_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-02-26_22-25-16_20_00sec_-14_90C_LIGHT_0164_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1830* 10 40 00.37 +12 36 55.4 10.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6830,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1830 10.06CV 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/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20.00sec_-14.90C_LIGHT_0162.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:40:00.37 +12:36:55.4 ;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_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1830* 10 50 19.27 +10 44 32.0 11.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6830,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1830 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20.00sec_-14.90C_LIGHT_0162.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:50:19.27 +10:44:32.0 ;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_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1830* 10 10 30.35 +13 46 50.4 11.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6830,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1830 11.63CV 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/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20.00sec_-14.90C_LIGHT_0162.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:10:30.35 +13:46:50.4 ;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_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1830* 10 33 34.90 +13 52 47.9 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6830,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1830 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/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20.00sec_-14.90C_LIGHT_0162.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:33:34.90 +13:52:47.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1830* 10 09 42.53 +18 45 25.9 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6830,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1830 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/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20.00sec_-14.90C_LIGHT_0162.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:42.53 +18:45:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1830* 10 16 25.55 +17 41 44.8 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6830,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1830 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20.00sec_-14.90C_LIGHT_0162.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:16:25.55 +17:41:44.8 ;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_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1830* 10 43 31.92 +11 28 14.9 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6830,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1830 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20.00sec_-14.90C_LIGHT_0162.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:43:31.92 +11:28:14.9 ;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_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1830* 10 58 32.02 +11 36 29.5 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.6830,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1830 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/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Leo-05-Q1b1x1_222729_TTUQ1b1x1_20103_dAUi519P/fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20.00sec_-14.90C_LIGHT_0162.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:58:32.02 +11:36:29.5 ;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_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-23-45_20_00sec_-14_90C_LIGHT_0162_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-26_22-22-50_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6919,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1919 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/Cam-01-Q1b1x1_2025-12-23_02-44-02_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-01-Q1b1x1_223720_TTUQ1b1x1_29996_dWXCyDPU/fd_Cam-01-Q1b1x1_2026-02-26_22-35-42_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-01-Q1b1x1_223720_TTUQ1b1x1_29996_dWXCyDPU/fd_Cam-01-Q1b1x1_2026-02-26_22-36-35_20.00sec_-14.90C_LIGHT_0173.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:29:23.13 +85:27:08.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-02-26_22-36-35_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-02-26_22-35-42_20_00sec_-15_00C_LIGHT_0172_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-02-26_22-36-35_20_00sec_-14_90C_LIGHT_0173_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-02-26_22-35-42_20_00sec_-15_00C_LIGHT_0172_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6919,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1919 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/Cam-01-Q1b1x1_2025-12-23_02-44-02_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-01-Q1b1x1_223720_TTUQ1b1x1_29996_dWXCyDPU/fd_Cam-01-Q1b1x1_2026-02-26_22-35-42_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-01-Q1b1x1_223720_TTUQ1b1x1_29996_dWXCyDPU/fd_Cam-01-Q1b1x1_2026-02-26_22-36-35_20.00sec_-14.90C_LIGHT_0173.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:17:17.72 +79:26:56.1 ;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_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-02-26_22-36-35_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-02-26_22-35-42_20_00sec_-15_00C_LIGHT_0172_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-02-26_22-36-35_20_00sec_-14_90C_LIGHT_0173_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-02-26_22-35-42_20_00sec_-15_00C_LIGHT_0172_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.6941,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.1941 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/Cam-02-Q1b1x1_2025-12-23_04-00-21_20.00sec_-15.00C_LIGHT_0526.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-02-Q1b1x1_224020_TTUQ1b1x1_22327_wTDPbpXZ/fd_Cam-02-Q1b1x1_2026-02-26_22-38-58_20.00sec_-14.90C_LIGHT_0175.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-02-Q1b1x1_224020_TTUQ1b1x1_22327_wTDPbpXZ/fd_Cam-02-Q1b1x1_2026-02-26_22-39-40_20.00sec_-15.00C_LIGHT_0176.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:10:23.69 +86:04:24.3 ;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_Cam-02-Q1b1x1_2025-12-23_04-00-21_20_00sec_-15_00C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Cam-02-Q1b1x1_2026-02-26_22-39-40_20_00sec_-15_00C_LIGHT_0176_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-02-Q1b1x1_2025-12-23_04-00-21_20_00sec_-15_00C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Cam-02-Q1b1x1_2026-02-26_22-38-58_20_00sec_-14_90C_LIGHT_0175_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-02-Q1b1x1_2025-12-23_04-00-21_20_00sec_-15_00C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Cam-02-Q1b1x1_2026-02-26_22-39-40_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-02-Q1b1x1_2025-12-23_04-00-21_20_00sec_-15_00C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Cam-02-Q1b1x1_2026-02-26_22-38-58_20_00sec_-14_90C_LIGHT_0175_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0225225+783327,2461098.7010,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0225225+783327 20260227.2010 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/Cep-02-Q1b1x1_2025-12-22_22-28-20_20.00sec_-15.00C_LIGHT_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-02-Q1b1x1_225020_TTUQ1b1x1_16283_ZX0izrbQ/fd_Cep-02-Q1b1x1_2026-02-26_22-48-58_20.00sec_-14.90C_LIGHT_0183.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-02-Q1b1x1_225020_TTUQ1b1x1_16283_ZX0izrbQ/fd_Cep-02-Q1b1x1_2026-02-26_22-49-39_20.00sec_-15.00C_LIGHT_0184.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:25:18.65 +78:33:28.6 ;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_Cep-02-Q1b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q1b1x1_2026-02-26_22-49-39_20_00sec_-15_00C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-02-Q1b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q1b1x1_2026-02-26_22-48-58_20_00sec_-14_90C_LIGHT_0183_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q1b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q1b1x1_2026-02-26_22-49-39_20_00sec_-15_00C_LIGHT_0184_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q1b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q1b1x1_2026-02-26_22-48-58_20_00sec_-14_90C_LIGHT_0183_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 566419672817945088,2461098.7010,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 566419672817945088 20260227.2010 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q1b1x1_2025-12-22_22-28-20_20.00sec_-15.00C_LIGHT_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-02-Q1b1x1_225020_TTUQ1b1x1_16283_ZX0izrbQ/fd_Cep-02-Q1b1x1_2026-02-26_22-48-58_20.00sec_-14.90C_LIGHT_0183.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cep-02-Q1b1x1_225020_TTUQ1b1x1_16283_ZX0izrbQ/fd_Cep-02-Q1b1x1_2026-02-26_22-49-39_20.00sec_-15.00C_LIGHT_0184.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:20.23 +80:32:44.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-02-Q1b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q1b1x1_2026-02-26_22-49-39_20_00sec_-15_00C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-02-Q1b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q1b1x1_2026-02-26_22-48-58_20_00sec_-14_90C_LIGHT_0183_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q1b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q1b1x1_2026-02-26_22-49-39_20_00sec_-15_00C_LIGHT_0184_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q1b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q1b1x1_2026-02-26_22-48-58_20_00sec_-14_90C_LIGHT_0183_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2024 2461098.7024 13.73 04:52:35.38 +73:49:21.6
137.70335 18.36257 galactic Cam Second-epoch detections are separated by 5.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | NSVS J0452402+734843 | 04:52:39.79 +73:48:44.9 (Gaia DR3) | L: (local) | 95.000000000000 (local) | Gaia3var=VARIABLE SpType: M2 1947AnDea...5....1L DO 28604
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0452402+734843,2461098.7024,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0452402+734843 20260227.2024 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/Cam-03-Q1b1x1_2025-12-23_01-09-01_20.00sec_-15.00C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-03-Q1b1x1_225220_TTUQ1b1x1_6596_pksaNGQ0/fd_Cam-03-Q1b1x1_2026-02-26_22-50-54_20.00sec_-15.00C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-03-Q1b1x1_225220_TTUQ1b1x1_6596_pksaNGQ0/fd_Cam-03-Q1b1x1_2026-02-26_22-51-44_20.00sec_-15.00C_LIGHT_0186.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:52:35.38 +73:49:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-03-Q1b1x1_2025-12-23_01-09-01_20_00sec_-15_00C_LIGHT_0358_fits__*pix.png resample_wcs_fd_Cam-03-Q1b1x1_2026-02-26_22-51-44_20_00sec_-15_00C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-03-Q1b1x1_2025-12-23_01-09-01_20_00sec_-15_00C_LIGHT_0358_fits__*pix.png resample_wcs_fd_Cam-03-Q1b1x1_2026-02-26_22-50-54_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-03-Q1b1x1_2025-12-23_01-09-01_20_00sec_-15_00C_LIGHT_0358_fits__*pix.png resample_wcs_fd_Cam-03-Q1b1x1_2026-02-26_22-51-44_20_00sec_-15_00C_LIGHT_0186_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-03-Q1b1x1_2025-12-23_01-09-01_20_00sec_-15_00C_LIGHT_0358_fits__*pix.png resample_wcs_fd_Cam-03-Q1b1x1_2026-02-26_22-50-54_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2047 2461098.7047 12.81 07:57:58.42 +75:07:15.1
139.50687 30.40527 galactic Cam Second-epoch detections are separated by 0.5" 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 1135779980891494528 | 07:57:55.85 +75:07:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.569+/-0.034 (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
Gaia DR3 1135779980891494528,2461098.7047,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1135779980891494528 20260227.2047 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-04-Q1b1x1_2025-12-23_04-07-50_20.00sec_-15.00C_LIGHT_0534.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-04-Q1b1x1_225535_TTUQ1b1x1_13719_wUugeks1/fd_Cam-04-Q1b1x1_2026-02-26_22-54-16_20.00sec_-15.00C_LIGHT_0188.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cam-04-Q1b1x1_225535_TTUQ1b1x1_13719_wUugeks1/fd_Cam-04-Q1b1x1_2026-02-26_22-54-54_20.00sec_-14.90C_LIGHT_0189.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:57:58.42 +75:07:15.1 ;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_Cam-04-Q1b1x1_2025-12-23_04-07-50_20_00sec_-15_00C_LIGHT_0534_fits__*pix.png resample_wcs_fd_Cam-04-Q1b1x1_2026-02-26_22-54-54_20_00sec_-14_90C_LIGHT_0189_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-04-Q1b1x1_2025-12-23_04-07-50_20_00sec_-15_00C_LIGHT_0534_fits__*pix.png resample_wcs_fd_Cam-04-Q1b1x1_2026-02-26_22-54-16_20_00sec_-15_00C_LIGHT_0188_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-04-Q1b1x1_2025-12-23_04-07-50_20_00sec_-15_00C_LIGHT_0534_fits__*pix.png resample_wcs_fd_Cam-04-Q1b1x1_2026-02-26_22-54-54_20_00sec_-14_90C_LIGHT_0189_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-04-Q1b1x1_2025-12-23_04-07-50_20_00sec_-15_00C_LIGHT_0534_fits__*pix.png resample_wcs_fd_Cam-04-Q1b1x1_2026-02-26_22-54-16_20_00sec_-15_00C_LIGHT_0188_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7088,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2088 9.86CV 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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20.00sec_-15.00C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:11:13.39 -17:53:15.5 ;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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7088,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2088 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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20.00sec_-15.00C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:12:21.10 -13:53:40.7 ;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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2088 2461098.7088 12.12 12:51:09.74 -18:41:08.3
302.84090 44.18606 galactic Crv Second-epoch detections are separated by 0.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J192.7899-18.6833 | 12:51:09.78 -18:41:08.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.387+/-0.033 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192.7899-18.6833,2461098.7088,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J192.7899-18.6833 20260227.2088 12.12CV 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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20.00sec_-15.00C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:51:09.74 -18:41:08.3 ;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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2088 2461098.7088 13.10 12:29:01.15 -22:23:24.2
296.14351 40.18601 galactic Crv Second-epoch detections are separated by 1.7" and 7.5 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 | 12:29:01.15 -22:23:24.2 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.033 (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,2461098.7088,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2088 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20.00sec_-15.00C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:29:01.15 -22:23:24.2 ;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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
U Crv,2461098.7088,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
U Crv 20260227.2088 11.05CV 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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20.00sec_-15.00C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:35:01.96 -18:27:38.8 ;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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2088 2461098.7088 12.46 12:49:39.34 -19:11:33.3
302.35009 43.67715 galactic Crv Second-epoch detections are separated by 1.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J192.4141-19.1925 | 12:49:39.40 -19:11:33.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.334+/-0.037 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192.4141-19.1925,2461098.7088,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J192.4141-19.1925 20260227.2088 12.46CV 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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Crv-01-Q1b1x1_230150_TTUQ1b1x1_21085_nk0fpDLt/fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20.00sec_-15.00C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:49:39.34 -19:11:33.3 ;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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-01-06_20_00sec_-15_00C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crv-01-Q1b1x1_2026-02-26_23-00-00_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2168* 10 55 39.80 +71 52 09.2 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VX UMa,2461098.7168,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VX UMa 20260227.2168 11.88CV 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/UMa-01-Q1b1x1_2025-12-23_04-16-13_20.00sec_-15.00C_LIGHT_0542.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2025-12-23_04-16-58_20.00sec_-15.00C_LIGHT_0543.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_UMa-01-Q1b1x1_231320_TTUQ1b1x1_2960_GzIvTsNk/fd_UMa-01-Q1b1x1_2026-02-26_23-11-30_20.00sec_-15.00C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_UMa-01-Q1b1x1_231320_TTUQ1b1x1_2960_GzIvTsNk/fd_UMa-01-Q1b1x1_2026-02-26_23-12-31_20.00sec_-14.90C_LIGHT_0206.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:55:39.80 +71:52:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-01-Q1b1x1_2025-12-23_04-16-13_20_00sec_-15_00C_LIGHT_0542_fits__*pix.png resample_wcs_fd_UMa-01-Q1b1x1_2026-02-26_23-12-31_20_00sec_-14_90C_LIGHT_0206_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-01-Q1b1x1_2025-12-23_04-16-13_20_00sec_-15_00C_LIGHT_0542_fits__*pix.png resample_wcs_fd_UMa-01-Q1b1x1_2026-02-26_23-11-30_20_00sec_-15_00C_LIGHT_0205_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-01-Q1b1x1_2025-12-23_04-16-13_20_00sec_-15_00C_LIGHT_0542_fits__*pix.png resample_wcs_fd_UMa-01-Q1b1x1_2026-02-26_23-12-31_20_00sec_-14_90C_LIGHT_0206_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-01-Q1b1x1_2025-12-23_04-16-13_20_00sec_-15_00C_LIGHT_0542_fits__*pix.png resample_wcs_fd_UMa-01-Q1b1x1_2026-02-26_23-11-30_20_00sec_-15_00C_LIGHT_0205_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 11.19 18:07:29.04 +64:52:17.2
94.46563 29.00375 galactic Dra Second-epoch detections are separated by 4.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161500123448459264 | 18:07:30.56 +64:52:21.4 (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 2161500123448459264,2461098.7226,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161500123448459264 20260227.2226 11.19CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:29.04 +64:52:17.2 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 10.47 18:06:47.09 +64:57:01.9
94.55227 29.08128 galactic Dra Second-epoch detections are separated by 3.7" and 6.9 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 2161502734788130688 | 18:06:48.44 +64:57:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161502734788130688,2461098.7226,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161502734788130688 20260227.2226 10.47CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:06:47.09 +64:57:01.9 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 10.87 18:07:58.48 +65:05:12.1
94.71415 28.96176 galactic Dra Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161498542900078848 | 18:07:59.46 +65:05:14.3 (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 2161498542900078848,2461098.7226,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161498542900078848 20260227.2226 10.87CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:58.48 +65:05:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 11.76 18:08:00.38 +64:54:53.7
94.51822 28.95043 galactic Dra Second-epoch detections are separated by 3.9" and 6.9 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 2161490159123804160 | 18:08:01.88 +64:54:58.3 (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 2161490159123804160,2461098.7226,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161490159123804160 20260227.2226 11.76CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:00.38 +64:54:53.7 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 12.38 18:08:00.38 +65:00:23.2
94.62271 28.95473 galactic Dra Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161496751897920384 | 18:08:01.36 +65:00:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161496751897920384,2461098.7226,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161496751897920384 20260227.2226 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:00.38 +65:00:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2226 2461098.7226 12.46 18:07:12.60 +64:59:30.2
94.60156 29.03812 galactic Dra Second-epoch detections are separated by 3.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2161503147105088896 | 18:07:13.76 +64:59:33.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2161503147105088896,2461098.7226,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161503147105088896 20260227.2226 12.46CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:12.60 +64:59:30.2 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7226,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2226 12.72CV 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:06:32.40 +64:52:55.2 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 2161480023001051136,2461098.7226,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2161480023001051136 20260227.2226 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:06:30.00 +64:50:14.3 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7226,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2226 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:07.36 +64:50:20.4 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7226,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2226 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:07:55.90 +64:49:39.3 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7226,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2226 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/Dra-04-Q1b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20.00sec_-15.00C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-04-Q1b1x1_232135_TTUQ1b1x1_20179_M1bdXgTT/fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20.00sec_-14.90C_LIGHT_0215.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:08:27.23 +64:51:53.6 ;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_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-20-50_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q1b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q1b1x1_2026-02-26_23-19-54_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
X Dra,2461098.7238,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
X Dra 20260227.2238 12.69CV 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/Dra-05-Q1b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-05-Q1b1x1_232320_TTUQ1b1x1_585_ZNzmUO0Y/fd_Dra-05-Q1b1x1_2026-02-26_23-21-40_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-05-Q1b1x1_232320_TTUQ1b1x1_585_ZNzmUO0Y/fd_Dra-05-Q1b1x1_2026-02-26_23-22-39_20.00sec_-14.90C_LIGHT_0217.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:06:52.88 +66:09:24.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q1b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q1b1x1_2026-02-26_23-22-39_20_00sec_-14_90C_LIGHT_0217_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q1b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q1b1x1_2026-02-26_23-21-40_20_00sec_-15_00C_LIGHT_0216_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q1b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q1b1x1_2026-02-26_23-22-39_20_00sec_-14_90C_LIGHT_0217_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q1b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q1b1x1_2026-02-26_23-21-40_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2312* 10 52 03.14 -33 27 15.6 13.4 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461098.7312,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2312 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/Hya-15-Q1b1x1_2026-01-21_03-08-56_20.00sec_-15.00C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-15-Q1b1x1_233350_TTUQ1b1x1_23675_3ZPbBdsr/fd_Hya-15-Q1b1x1_2026-02-26_23-32-21_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-15-Q1b1x1_233350_TTUQ1b1x1_23675_3ZPbBdsr/fd_Hya-15-Q1b1x1_2026-02-26_23-33-05_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:52:03.14 -33:27:15.6 ;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_Hya-15-Q1b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q1b1x1_2026-02-26_23-33-05_20_00sec_-15_00C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-15-Q1b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q1b1x1_2026-02-26_23-32-21_20_00sec_-14_90C_LIGHT_0227_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-15-Q1b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q1b1x1_2026-02-26_23-33-05_20_00sec_-15_00C_LIGHT_0228_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-15-Q1b1x1_2026-01-21_03-08-56_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png resample_wcs_fd_Hya-15-Q1b1x1_2026-02-26_23-32-21_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2325 2461098.7325 12.29 17:59:49.00 +58:59:55.5
87.68290 29.55293 galactic Dra Second-epoch detections are separated by 1.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1422766538809968640 | 17:59:49.04 +58:59:56.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.482+/-0.028 (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
Gaia DR3 1422766538809968640,2461098.7325,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1422766538809968640 20260227.2325 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-07-Q1b1x1_2025-12-23_06-37-17_20.00sec_-15.00C_LIGHT_0702.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-07-Q1b1x1_2025-12-23_06-38-13_20.00sec_-15.00C_LIGHT_0703.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-07-Q1b1x1_233550_TTUQ1b1x1_856_7Q93uUri/fd_Dra-07-Q1b1x1_2026-02-26_23-34-06_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-07-Q1b1x1_233550_TTUQ1b1x1_856_7Q93uUri/fd_Dra-07-Q1b1x1_2026-02-26_23-35-07_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:59:49.00 +58:59:55.5 ;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_Dra-07-Q1b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q1b1x1_2026-02-26_23-35-07_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-07-Q1b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q1b1x1_2026-02-26_23-34-06_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-07-Q1b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q1b1x1_2026-02-26_23-35-07_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-07-Q1b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q1b1x1_2026-02-26_23-34-06_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2356 2461098.7356 13.03 13:04:12.86 -30:51:49.3
306.16247 31.92790 galactic Cen Second-epoch detections are separated by 3.6" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6181046658701355392 | 13:04:13.86 -30:51:59.3 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 6181046658701355392,2461098.7356,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6181046658701355392 20260227.2356 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/Hya-12-Q1b1x1_2026-01-21_03-43-02_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:04:12.86 -30:51:49.3 ;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_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2356 2461098.7356 12.57 12:48:23.01 -30:16:58.0
302.14933 32.58433 galactic Cen Second-epoch detections are separated by 0.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6184866190297899264 | 12:48:23.03 -30:16:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.256+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 6184866190297899264,2461098.7356,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6184866190297899264 20260227.2356 12.57CV 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/Hya-12-Q1b1x1_2026-01-21_03-43-02_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-12-Q1b1x1_2026-01-21_03-43-47_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:48:23.01 -30:16:58.0 ;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_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2356 2461098.7356 11.38 12:43:12.38 -29:58:12.2
300.80940 32.86777 galactic Hya Second-epoch detections are separated by 0.7" and 7.2 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 3470783898195234176 | 12:43:12.43 -29:58:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.032 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3470783898195234176,2461098.7356,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3470783898195234176 20260227.2356 11.38CV 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/Hya-12-Q1b1x1_2026-01-21_03-43-02_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-12-Q1b1x1_2026-01-21_03-43-47_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:43:12.38 -29:58:12.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2356 2461098.7356 12.12 12:51:38.28 -30:04:03.6
302.98342 32.80406 galactic Hya Second-epoch detections are separated by 1.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6184799154448539904 | 12:51:38.24 -30:04:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.667+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 6184799154448539904,2461098.7356,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6184799154448539904 20260227.2356 12.12CV 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/Hya-12-Q1b1x1_2026-01-21_03-43-02_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-12-Q1b1x1_2026-01-21_03-43-47_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:51:38.28 -30:04:03.6 ;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_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2356 2461098.7356 11.84 13:01:58.22 -26:48:16.6
305.83740 36.00771 galactic Hya Second-epoch detections are separated by 0.2" and 7.8 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 6187270478630310912 | 13:01:58.20 -26:48:15.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.788+/-0.039 (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
Gaia DR3 6187270478630310912,2461098.7356,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6187270478630310912 20260227.2356 11.84CV 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/Hya-12-Q1b1x1_2026-01-21_03-43-02_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-12-Q1b1x1_2026-01-21_03-43-47_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-12-Q1b1x1_234020_TTUQ1b1x1_21015_Stv3yBN0/fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:01:58.22 -26:48:16.6 ;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_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-39-32_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-12-Q1b1x1_2026-01-21_03-43-02_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-12-Q1b1x1_2026-02-26_23-38-46_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7400,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2400 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/Dra-09-Q1b1x1_2025-12-23_05-11-49_20.00sec_-15.00C_LIGHT_0606.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-09-Q1b1x1_234620_TTUQ1b1x1_32419_zGefVI0V/fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20.00sec_-14.90C_LIGHT_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-09-Q1b1x1_234620_TTUQ1b1x1_32419_zGefVI0V/fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20.00sec_-15.00C_LIGHT_0241.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:57:34.32 +58:37:29.2 ;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_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20_00sec_-15_00C_LIGHT_0241_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20_00sec_-14_90C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20_00sec_-15_00C_LIGHT_0241_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20_00sec_-14_90C_LIGHT_0240_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7400,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2400 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/Dra-09-Q1b1x1_2025-12-23_05-11-49_20.00sec_-15.00C_LIGHT_0606.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-09-Q1b1x1_234620_TTUQ1b1x1_32419_zGefVI0V/fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20.00sec_-14.90C_LIGHT_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-09-Q1b1x1_234620_TTUQ1b1x1_32419_zGefVI0V/fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20.00sec_-15.00C_LIGHT_0241.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:10:42.42 +55:52:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20_00sec_-15_00C_LIGHT_0241_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20_00sec_-14_90C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20_00sec_-15_00C_LIGHT_0241_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20_00sec_-14_90C_LIGHT_0240_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7400,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2400 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-09-Q1b1x1_2025-12-23_05-11-49_20.00sec_-15.00C_LIGHT_0606.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-09-Q1b1x1_234620_TTUQ1b1x1_32419_zGefVI0V/fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20.00sec_-14.90C_LIGHT_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-09-Q1b1x1_234620_TTUQ1b1x1_32419_zGefVI0V/fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20.00sec_-15.00C_LIGHT_0241.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:43:26.99 +49:15:42.6 ;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_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20_00sec_-15_00C_LIGHT_0241_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20_00sec_-14_90C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20_00sec_-15_00C_LIGHT_0241_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20_00sec_-14_90C_LIGHT_0240_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461098.7400,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260227.2400 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/Dra-09-Q1b1x1_2025-12-23_05-11-49_20.00sec_-15.00C_LIGHT_0606.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-09-Q1b1x1_234620_TTUQ1b1x1_32419_zGefVI0V/fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20.00sec_-14.90C_LIGHT_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-09-Q1b1x1_234620_TTUQ1b1x1_32419_zGefVI0V/fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20.00sec_-15.00C_LIGHT_0241.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:56:40.37 +57:11:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20_00sec_-15_00C_LIGHT_0241_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20_00sec_-14_90C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-42_20_00sec_-15_00C_LIGHT_0241_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-02-26_23-45-08_20_00sec_-14_90C_LIGHT_0240_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2410 2461098.7410 12.45 17:46:24.66 +48:52:56.1
75.82625 30.48812 galactic Her Second-epoch detections are separated by 0.3" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1363933419658692608 | 17:46:25.11 +48:52:51.8 (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 02 27.2410* 17 46 24.66 +48 52 56.1 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1363933419658692608,2461098.7410,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1363933419658692608 20260227.2410 12.45CV 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/Dra-10-Q1b1x1_2026-01-09_03-16-10_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-10-Q1b1x1_234805_TTUQ1b1x1_7960_JTOXU5U5/fd_Dra-10-Q1b1x1_2026-02-26_23-46-30_20.00sec_-14.90C_LIGHT_0242.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Dra-10-Q1b1x1_234805_TTUQ1b1x1_7960_JTOXU5U5/fd_Dra-10-Q1b1x1_2026-02-26_23-47-15_20.00sec_-15.00C_LIGHT_0243.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:46:24.66 +48:52:56.1 ;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_Dra-10-Q1b1x1_2026-01-09_03-16-10_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Dra-10-Q1b1x1_2026-02-26_23-47-15_20_00sec_-15_00C_LIGHT_0243_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-10-Q1b1x1_2026-01-09_03-16-10_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Dra-10-Q1b1x1_2026-02-26_23-46-30_20_00sec_-14_90C_LIGHT_0242_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-10-Q1b1x1_2026-01-09_03-16-10_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Dra-10-Q1b1x1_2026-02-26_23-47-15_20_00sec_-15_00C_LIGHT_0243_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-10-Q1b1x1_2026-01-09_03-16-10_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Dra-10-Q1b1x1_2026-02-26_23-46-30_20_00sec_-14_90C_LIGHT_0242_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2437 2461098.7437 13.38 12:15:51.55 +47:05:52.2
139.88664 68.84192 galactic CVn Second-epoch detections are separated by 0.9" and 7.1 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 1545183036711576064 | 12:15:51.29 +47:06:20.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1545183036711576064,2461098.7437,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1545183036711576064 20260227.2437 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/UMa-11-Q1b1x1_2025-12-23_05-15-12_20.00sec_-14.90C_LIGHT_0610.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_UMa-11-Q1b1x1_235220_TTUQ1b1x1_4356_SPY4C1bq/fd_UMa-11-Q1b1x1_2026-02-26_23-50-20_20.00sec_-14.90C_LIGHT_0246.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_UMa-11-Q1b1x1_235220_TTUQ1b1x1_4356_SPY4C1bq/fd_UMa-11-Q1b1x1_2026-02-26_23-51-02_20.00sec_-15.00C_LIGHT_0247.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:15:51.55 +47:05:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-11-Q1b1x1_2025-12-23_05-15-12_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png resample_wcs_fd_UMa-11-Q1b1x1_2026-02-26_23-51-02_20_00sec_-15_00C_LIGHT_0247_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-11-Q1b1x1_2025-12-23_05-15-12_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png resample_wcs_fd_UMa-11-Q1b1x1_2026-02-26_23-50-20_20_00sec_-14_90C_LIGHT_0246_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-11-Q1b1x1_2025-12-23_05-15-12_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png resample_wcs_fd_UMa-11-Q1b1x1_2026-02-26_23-51-02_20_00sec_-15_00C_LIGHT_0247_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-11-Q1b1x1_2025-12-23_05-15-12_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png resample_wcs_fd_UMa-11-Q1b1x1_2026-02-26_23-50-20_20_00sec_-14_90C_LIGHT_0246_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.2437 2461098.7437 11.94 12:15:51.34 +47:06:19.3
139.88022 68.83473 galactic CVn Second-epoch detections are separated by 0.3" and 7.3 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 1545183036711576064 | 12:15:51.29 +47:06:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.026 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1545183036711576064,2461098.7437,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1545183036711576064 20260227.2437 11.94CV 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/UMa-11-Q1b1x1_2025-12-23_05-15-12_20.00sec_-14.90C_LIGHT_0610.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-11-Q1b1x1_2025-12-23_05-15-52_20.00sec_-15.00C_LIGHT_0611.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_UMa-11-Q1b1x1_235220_TTUQ1b1x1_4356_SPY4C1bq/fd_UMa-11-Q1b1x1_2026-02-26_23-50-20_20.00sec_-14.90C_LIGHT_0246.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_UMa-11-Q1b1x1_235220_TTUQ1b1x1_4356_SPY4C1bq/fd_UMa-11-Q1b1x1_2026-02-26_23-51-02_20.00sec_-15.00C_LIGHT_0247.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:15:51.34 +47:06:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-11-Q1b1x1_2025-12-23_05-15-12_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png resample_wcs_fd_UMa-11-Q1b1x1_2026-02-26_23-51-02_20_00sec_-15_00C_LIGHT_0247_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-11-Q1b1x1_2025-12-23_05-15-12_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png resample_wcs_fd_UMa-11-Q1b1x1_2026-02-26_23-50-20_20_00sec_-14_90C_LIGHT_0246_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-11-Q1b1x1_2025-12-23_05-15-12_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png resample_wcs_fd_UMa-11-Q1b1x1_2026-02-26_23-51-02_20_00sec_-15_00C_LIGHT_0247_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-11-Q1b1x1_2025-12-23_05-15-12_20_00sec_-14_90C_LIGHT_0610_fits__*pix.png resample_wcs_fd_UMa-11-Q1b1x1_2026-02-26_23-50-20_20_00sec_-14_90C_LIGHT_0246_fits__*pix.png animation_v2.gif