Mean magnitude and position on the discovery images:
2026 01 18.0542 2461058.5542 14.10 21:30:37.54 +54:16:42.8
96.25904 2.15528 galactic Cyg Second-epoch detections are separated by 2.7" 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 J322.6410+54.2777 | 21:30:37.32 +54:16:36.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J322.6410+54.2777,2461058.5542,14.10,0.05,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
ATO J322.6410+54.2777 20260118.0542 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-02-Q1b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-02-Q1b1x1_220150_TTUQ1b1x1_1109_bbbb1VAK/fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_20.00sec_-14.90C_LIGHT_0006.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-02-Q1b1x1_220150_TTUQ1b1x1_1109_bbbb1VAK/fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20.00sec_-14.90C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:30:37.54 +54:16:42.8 ;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_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20_00sec_-14_90C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_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_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20_00sec_-14_90C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0542 2461058.5542 14.18 21:35:50.99 +53:29:12.6
96.28885 1.05143 galactic Cyg Second-epoch detections are separated by 3.8" 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 2174192816978711680 | 21:35:52.79 +53:29:32.9 (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 2174192816978711680,2461058.5542,14.18,0.05,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
Gaia DR3 2174192816978711680 20260118.0542 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-02-Q1b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-02-Q1b1x1_220150_TTUQ1b1x1_1109_bbbb1VAK/fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_20.00sec_-14.90C_LIGHT_0006.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-02-Q1b1x1_220150_TTUQ1b1x1_1109_bbbb1VAK/fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20.00sec_-14.90C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:35:50.99 +53:29:12.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20_00sec_-14_90C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_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_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20_00sec_-14_90C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0542 2461058.5542 14.02 21:57:46.90 +51:07:59.9
97.34875 -2.90318 galactic Cyg Second-epoch detections are separated by 0.8" 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 J329.4594+51.1214 | 21:57:49.38 +51:07:40.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J329.4594+51.1214,2461058.5542,14.02,0.05,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 J329.4594+51.1214 20260118.0542 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-02-Q1b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-02-Q1b1x1_220150_TTUQ1b1x1_1109_bbbb1VAK/fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_20.00sec_-14.90C_LIGHT_0006.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-02-Q1b1x1_220150_TTUQ1b1x1_1109_bbbb1VAK/fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20.00sec_-14.90C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:57:46.90 +51:07:59.9 ;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_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20_00sec_-14_90C_LIGHT_0007_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_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_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-18-19_20_00sec_-14_90C_LIGHT_0007_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-17_19-17-19_20_00sec_-14_90C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 14.03 20:40:05.28 +45:25:58.9
84.26113 2.27772 galactic Cyg Second-epoch detections are separated by 3.1" 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 | ATO J310.0220+45.4330 | 20:40:04.98 +45:26:43.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.473+/-0.042 (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
ATO J310.0220+45.4330,2461058.5515,14.03,0.05,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
ATO J310.0220+45.4330 20260118.0515 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:40:05.28 +45:25:58.9 ;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_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 13.80 21:05:34.84 +44:54:42.6
86.73848 -1.50544 galactic Cyg Second-epoch detections are separated by 5.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2162618429876014976 | 21:05:35.51 +44:54:14.4 (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 2162618429876014976,2461058.5515,13.80,0.05,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
Gaia DR3 2162618429876014976 20260118.0515 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:05:34.84 +44:54:42.6 ;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_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 13.75 20:27:24.18 +48:16:23.0
85.26209 5.70810 galactic Cyg Second-epoch detections are separated by 2.8" 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 | ATO J306.8527+48.2834 | 20:27:22.72 +48:16:57.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J306.8527+48.2834,2461058.5515,13.75,0.05,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
ATO J306.8527+48.2834 20260118.0515 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:24.18 +48:16:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 13.84 21:00:50.92 +45:22:53.9
86.53469 -0.56984 galactic Cyg Second-epoch detections are separated by 4.1" and 6.8 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 J315.2160+45.3783 | 21:00:50.92 +45:22:53.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J315.2160+45.3783,2461058.5515,13.84,0.05,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
ATO J315.2160+45.3783 20260118.0515 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:50.92 +45:22:53.9 ;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_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 13.96 21:06:10.82 +47:03:34.5
88.40071 -0.14112 galactic Cyg Second-epoch detections are separated by 5.5" and 6.1 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 | Large-amplitude variable Gaia DR2 2165133184747940096 | 21:06:12.76 +47:04:01.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2165133184747940096,2461058.5515,13.96,0.05,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
Large-amplitude variable Gaia DR2 2165133184747940096 20260118.0515 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:06:10.82 +47:03:34.5 ;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_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 13.96 20:19:30.56 +47:52:22.9
84.17907 6.56781 galactic Cyg Second-epoch detections are separated by 7.7" 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 J304.8770+47.8717 | 20:19:30.56 +47:52:22.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.8770+47.8717,2461058.5515,13.96,0.05,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
ATO J304.8770+47.8717 20260118.0515 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:30.56 +47:52:22.9 ;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_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 13.90 20:20:51.91 +44:52:16.5
81.81278 4.69154 galactic Cyg Second-epoch detections are separated by 3.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2081399601861363712 | 20:20:48.54 +44:52:01.8 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2081399601861363712,2461058.5515,13.90,0.05,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 2081399601861363712 20260118.0515 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:51.91 +44:52:16.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 14.18 20:29:57.67 +48:26:06.8
85.64235 5.45574 galactic Cyg Second-epoch detections are separated by 0.5" 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 J307.4795+48.4255 | 20:29:57.82 +48:25:25.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J307.4795+48.4255,2461058.5515,14.18,0.05,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
ATO J307.4795+48.4255 20260118.0515 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:29:57.67 +48:26:06.8 ;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_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0515 2461058.5515 11.35 19:43:00.86 +40:57:34.7
74.82162 8.56505 galactic Cyg Second-epoch detections are separated by 0.8" and 6.8 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 J295.7383+40.9608 | 19:43:00.92 +40:57:35.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5/8III/IV 2016A&A...594A..39F KIC 5719468 J-Ks=0.136+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.7383+40.9608,2461058.5515,11.35,0.05,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
ATO J295.7383+40.9608 20260118.0515 11.35CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-03-Q1b1x1_2025-12-26_19-02-10_20.00sec_-15.00C_LIGHT_0003.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20.00sec_-15.00C_LIGHT_0002.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-03-Q1b1x1_220926_TTUQ1b1x1_4396_otGvDAyU/fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20.00sec_-15.00C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:43:00.86 +40:57:34.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-14-29_20_00sec_-15_00C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q1b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q1b1x1_2026-01-17_19-13-30_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1868 2461058.6868 14.47 04:37:38.17 -04:53:16.3
201.07081 -31.84638 galactic Eri Second-epoch detections are separated by 5.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3201153719731612544 | 04:37:38.17 -04:53:16.3 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.1868* 04 37 38.17 -04 53 16.3 14.5 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
Large-amplitude variable Gaia DR2 3201153719731612544,2461058.6868,14.47,0.05,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
Large-amplitude variable Gaia DR2 3201153719731612544 20260118.1868 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Eri-04-Q1b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Eri-04-Q1b1x1_235557_TTUQ1b1x1_6106_QA4h0YY2/fd_Eri-04-Q1b1x1_2026-01-17_22-28-25_20.00sec_-15.00C_LIGHT_0154.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Eri-04-Q1b1x1_235557_TTUQ1b1x1_6106_QA4h0YY2/fd_Eri-04-Q1b1x1_2026-01-17_22-29-14_20.00sec_-15.00C_LIGHT_0155.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:38.17 -04:53:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q1b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Eri-04-Q1b1x1_2026-01-17_22-29-14_20_00sec_-15_00C_LIGHT_0155_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q1b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Eri-04-Q1b1x1_2026-01-17_22-28-25_20_00sec_-15_00C_LIGHT_0154_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q1b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Eri-04-Q1b1x1_2026-01-17_22-29-14_20_00sec_-15_00C_LIGHT_0155_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q1b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Eri-04-Q1b1x1_2026-01-17_22-28-25_20_00sec_-15_00C_LIGHT_0154_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0942 2461058.5942 14.37 03:45:53.46 +45:34:41.3
152.05222 -7.20074 galactic Per Second-epoch detections are separated by 2.2" 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 J056.4720+45.5795 | 03:45:53.46 +45:34:41.3 (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 01 18.0942* 03 45 53.46 +45 34 41.3 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
ATO J056.4720+45.5795,2461058.5942,14.37,0.05,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
ATO J056.4720+45.5795 20260118.0942 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Per-02-Q1b1x1_220533_TTUQ1b1x1_17994_a8A0qb0S/fd_Per-02-Q1b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Per-02-Q1b1x1_220533_TTUQ1b1x1_17994_a8A0qb0S/fd_Per-02-Q1b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:53.46 +45:34:41.3 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-01-17_20-15-54_20_00sec_-14_90C_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_2026-01-17_20-15-07_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_2026-01-17_20-15-54_20_00sec_-14_90C_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_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0942 2461058.5942 13.73 04:21:55.66 +49:26:46.3
154.04030 -0.27589 galactic Per Second-epoch detections are separated by 0.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 270382450577169280 | 04:21:51.66 +49:26:20.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-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!
TCP 2026 01 18.0942* 04 21 55.66 +49 26 46.3 13.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 270382450577169280,2461058.5942,13.73,0.05,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
Gaia DR3 270382450577169280 20260118.0942 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Per-02-Q1b1x1_220533_TTUQ1b1x1_17994_a8A0qb0S/fd_Per-02-Q1b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Per-02-Q1b1x1_220533_TTUQ1b1x1_17994_a8A0qb0S/fd_Per-02-Q1b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:55.66 +49:26:46.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-01-17_20-15-54_20_00sec_-14_90C_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_2026-01-17_20-15-07_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_2026-01-17_20-15-54_20_00sec_-14_90C_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_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0942 2461058.5942 12.99 02:57:19.93 +41:48:02.2
146.71607 -15.18399 galactic Per Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:57:19.93 +41:48:02.2 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.031 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.0942* 02 57 19.93 +41 48 02.2 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.5942,12.99,0.05,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 20260118.0942 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Per-02-Q1b1x1_220533_TTUQ1b1x1_17994_a8A0qb0S/fd_Per-02-Q1b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Per-02-Q1b1x1_220533_TTUQ1b1x1_17994_a8A0qb0S/fd_Per-02-Q1b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:19.93 +41:48:02.2 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-01-17_20-15-54_20_00sec_-14_90C_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_2026-01-17_20-15-07_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_2026-01-17_20-15-54_20_00sec_-14_90C_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_2026-01-17_20-15-07_20_00sec_-15_00C_LIGHT_0027_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0942 2461058.5942 12.32 02:59:56.44 +42:50:08.3
146.63353 -14.04496 galactic Per Second-epoch detections are separated by 0.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 432457783133257856 | 02:59:56.40 +42:50:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.729+/-0.026 (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 01 18.0942* 02 59 56.44 +42 50 08.3 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 432457783133257856,2461058.5942,12.32,0.05,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
Gaia DR3 432457783133257856 20260118.0942 12.32CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-06_20.00sec_-14.90C_LIGHT_0322.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2025-12-23_00-38-53_20.00sec_-14.90C_LIGHT_0323.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Per-02-Q1b1x1_220533_TTUQ1b1x1_17994_a8A0qb0S/fd_Per-02-Q1b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Per-02-Q1b1x1_220533_TTUQ1b1x1_17994_a8A0qb0S/fd_Per-02-Q1b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:56.44 +42:50:08.3 ;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_Per-02-Q1b1x1_2025-12-23_00-38-06_20_00sec_-14_90C_LIGHT_0322_fits__*pix.png resample_wcs_fd_Per-02-Q1b1x1_2026-01-17_20-15-54_20_00sec_-14_90C_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_2026-01-17_20-15-07_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_2026-01-17_20-15-54_20_00sec_-14_90C_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_2026-01-17_20-15-07_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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.6076,14.16,0.05,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
target 20260118.1076 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:05:24.00 +02:58:20.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.6076,14.02,0.05,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
target 20260118.1076 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:44:48.25 +02:01:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 13.41 06:44:27.08 +01:07:07.6
211.13952 -1.04390 galactic Mon Second-epoch detections are separated by 5.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:44:27.08 +01:07:07.6 (user input) | T | P | (position from user input) SpType: G5IIb 2012A&A...543A.125G CoRoT 102734910
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.6076,13.41,0.05,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
target 20260118.1076 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:44:27.08 +01:07:07.6 ;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_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 13.05 06:43:29.65 +01:56:31.6
210.29770 -0.88073 galactic Mon Second-epoch detections are separated by 3.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3126022299206041600 | 06:43:30.50 +01:56:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1949AnHar.112....1C HD 289013
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 3126022299206041600,2461058.6076,13.05,0.05,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 3126022299206041600 20260118.1076 13.05CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:29.65 +01:56:31.6 ;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_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 12.26 06:34:26.94 +11:05:58.3
201.13003 1.32384 galactic Mon Second-epoch detections are separated by 1.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3328033307133056768 | 06:34:24.43 +11:06:11.4 (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 3328033307133056768,2461058.6076,12.26,0.05,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
Gaia DR3 3328033307133056768 20260118.1076 12.26CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:26.94 +11:05:58.3 ;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_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 12.84 06:44:25.88 +01:59:00.9
210.36776 -0.65348 galactic Mon Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.1090+01.9830 | 06:44:24.41 +01:58:38.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.1090+01.9830,2461058.6076,12.84,0.05,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
ATO J101.1090+01.9830 20260118.1076 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:44:25.88 +01:59:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 13.16 06:46:23.92 +01:22:31.0
211.13345 -0.49377 galactic Mon Second-epoch detections are separated by 1.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.5841+01.3784 | 06:46:21.89 +01:22:40.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9 1949AnHar.112....1C HD 289121
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 J101.5841+01.3784,2461058.6076,13.16,0.05,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
ATO J101.5841+01.3784 20260118.1076 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:46:23.92 +01:22:31.0 ;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_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 13.10 06:49:54.89 +01:05:44.9
211.78305 0.16082 galactic Mon Second-epoch detections are separated by 4.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3125683275966107136 | 06:49:55.50 +01:05:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F 1949AnHar.112....1C HD 289218
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 3125683275966107136,2461058.6076,13.10,0.05,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
Gaia DR3 3125683275966107136 20260118.1076 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:49:54.89 +01:05:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 13.47 06:43:19.44 +01:15:02.8
210.89339 -1.23432 galactic Mon Second-epoch detections are separated by 6.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3125836692194820352 | 06:43:16.59 +01:14:50.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A5 1949AnHar.112....1C HD 289043
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
Large-amplitude variable Gaia DR2 3125836692194820352,2461058.6076,13.47,0.05,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
Large-amplitude variable Gaia DR2 3125836692194820352 20260118.1076 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:19.44 +01:15:02.8 ;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_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 14.16 06:47:44.24 +08:25:14.7
205.01110 3.01285 galactic Mon Second-epoch detections are separated by 3.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.9333+08.4201 | 06:47:42.34 +08:25:31.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9333+08.4201,2461058.6076,14.16,0.05,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
ATO J101.9333+08.4201 20260118.1076 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:47:44.24 +08:25:14.7 ;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_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1076 2461058.6076 14.04 06:44:09.17 +01:28:16.3
210.79187 -0.94938 galactic Mon Second-epoch detections are separated by 4.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.0307+01.4656 | 06:44:09.17 +01:28:16.3 (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 J101.0307+01.4656,2461058.6076,14.04,0.05,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 J101.0307+01.4656 20260118.1076 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20.00sec_-15.00C_LIGHT_0047.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-01-Q1b1x1_232330_TTUQ1b1x1_27033_0a2zObSS/fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20.00sec_-14.90C_LIGHT_0048.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:44:09.17 +01:28:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-35-03_20_00sec_-14_90C_LIGHT_0048_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-17_20-34-23_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.6185,13.49,0.05,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
target 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:14.38 +11:24:57.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 13.08 06:53:07.07 +18:48:33.8
196.24292 8.81206 galactic Gem Second-epoch detections are separated by 1.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:53:07.07 +18:48:33.8 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.6185,13.08,0.05,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 20260118.1185 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:53:07.07 +18:48:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 12.31 06:39:03.68 +16:18:53.8
196.99620 4.70292 galactic Gem Second-epoch detections are separated by 4.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J099.7609+16.3201 | 06:39:03.03 +16:19:05.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.7609+16.3201,2461058.6185,12.31,0.05,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
ATO J099.7609+16.3201 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:39:03.68 +16:18:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 13.80 06:45:07.87 +09:02:31.2
204.16406 2.72131 galactic Mon Second-epoch detections are separated by 3.4" and 3.7 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 | FX Mon | 06:45:05.61 +09:02:18.2 (Gaia DR3) | M (local) | 428.500000000000 (local) | Gaia3var=VARIABLE SpType: M8 1978PASJ...30..657I [II78] 46
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
FX Mon,2461058.6185,13.80,0.05,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
FX Mon 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:45:07.87 +09:02:31.2 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 13.89 06:59:27.13 +08:58:50.0
205.81903 5.84932 galactic Mon Second-epoch detections are separated by 0.1" and 3.7 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 J104.8512+08.9749 | 06:59:27.13 +08:58:50.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7III (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.8512+08.9749,2461058.6185,13.89,0.05,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
ATO J104.8512+08.9749 20260118.1185 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:27.13 +08:58:50.0 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 14.18 06:45:59.85 +17:18:02.9
196.85924 6.62873 galactic Gem Second-epoch detections are separated by 4.1" 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 | ATO J101.5011+17.3010 | 06:45:59.85 +17:18:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.5011+17.3010,2461058.6185,14.18,0.05,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
ATO J101.5011+17.3010 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:45:59.85 +17:18:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 14.38 06:49:20.27 +12:31:04.4
201.52374 5.21370 galactic Gem 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 3351740495813090560 | 06:49:20.32 +12:31:46.9 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3351740495813090560,2461058.6185,14.38,0.05,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 3351740495813090560 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:49:20.27 +12:31:04.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 13.01 07:39:03.49 +17:27:13.5
202.18276 18.17432 galactic Gem Second-epoch detections are separated by 0.5" and 3.6 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 | 07:39:03.49 +17:27:13.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.618+/-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
target,2461058.6185,13.01,0.05,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
target 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:03.49 +17:27:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 13.15 07:37:40.36 +16:07:47.3
203.31429 17.33675 galactic Gem Second-epoch detections are separated by 0.4" and 3.6 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 | 07:37:40.36 +16:07:47.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.782+/-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
target,2461058.6185,13.15,0.05,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
target 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:40.36 +16:07:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 12.63 07:37:51.33 +18:18:29.8
201.23761 18.25216 galactic Gem Second-epoch detections are separated by 0.7" and 3.7 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 671404616451558144 | 07:37:51.38 +18:18:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.628+/-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 671404616451558144,2461058.6185,12.63,0.05,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 671404616451558144 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:51.33 +18:18:29.8 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 12.20 06:37:25.95 +09:17:01.2
203.08059 1.14134 galactic Mon Second-epoch detections are separated by 1.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J099.3552+09.2957 | 06:37:25.95 +09:17:01.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.306+/-0.030 (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 J099.3552+09.2957,2461058.6185,12.20,0.05,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
ATO J099.3552+09.2957 20260118.1185 12.20CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:25.95 +09:17:01.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 12.41 07:34:50.88 +18:51:22.6
200.41138 17.81516 galactic Gem Second-epoch detections are separated by 0.2" and 3.5 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 672248075012226816 | 07:34:50.90 +18:51:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.230+/-0.030 (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 672248075012226816,2461058.6185,12.41,0.05,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
Gaia DR3 672248075012226816 20260118.1185 12.41CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:34:50.88 +18:51:22.6 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 12.22 07:33:05.67 +18:22:13.0
200.70541 17.24055 galactic Gem Second-epoch detections are separated by 0.3" and 3.6 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 J113.2821+18.3690 | 07:33:05.71 +18:22:13.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.558+/-0.036 (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
ATO J113.2821+18.3690,2461058.6185,12.22,0.05,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 J113.2821+18.3690 20260118.1185 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:05.67 +18:22:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 13.22 07:31:35.60 +17:40:15.2
201.22474 16.63253 galactic Gem Second-epoch detections are separated by 3.2" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:31:35.60 +17:40:15.2 (user input) | T | P | (position from user input) J-Ks=0.626+/-0.027 (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,2461058.6185,13.22,0.05,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
target 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:31:35.60 +17:40:15.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 13.41 07:37:10.18 +18:16:34.2
201.20062 18.09000 galactic Gem Second-epoch detections are separated by 0.9" and 3.5 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 | 07:37:10.18 +18:16:34.2 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.6185,13.41,0.05,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
target 20260118.1185 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:10.18 +18:16:34.2 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1185 2461058.6185 13.23 07:37:51.07 +18:34:41.8
200.97604 18.35813 galactic Gem Second-epoch detections are separated by 0.7" and 3.5 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 J114.4630+18.5785 | 07:37:51.07 +18:34:41.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.339+/-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
ATO J114.4630+18.5785,2461058.6185,13.23,0.05,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
ATO J114.4630+18.5785 20260118.1185 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-05-Q1b1x1_2025-12-23_02-33-50_20.00sec_-14.90C_LIGHT_0438.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Gem-05-Q1b1x1_230328_TTUQ1b1x1_314_8lsNNm5I/fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20.00sec_-14.90C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:51.07 +18:34:41.8 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-50_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-17_20-50-13_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2117 2461058.7117 14.26 06:21:46.95 -05:38:12.8
214.60729 -9.15310 galactic Mon Second-epoch detections are separated by 5.3" 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 | target | 06:21:46.95 -05:38:12.8 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.7117,14.26,0.05,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 20260118.2117 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-04-Q1b1x1_2025-12-23_00-26-26_20.00sec_-14.90C_LIGHT_0310.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20.00sec_-14.90C_LIGHT_0190.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20.00sec_-15.00C_LIGHT_0191.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:46.95 -05:38:12.8 ;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_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2117 2461058.7117 13.01 06:31:25.62 -07:39:14.0
217.51403 -7.91190 galactic Mon Second-epoch detections are separated by 4.4" 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 3006859260510430592 | 06:31:27.74 -07:39:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3006859260510430592,2461058.7117,13.01,0.05,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
Gaia DR3 3006859260510430592 20260118.2117 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-04-Q1b1x1_2025-12-23_00-26-26_20.00sec_-14.90C_LIGHT_0310.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20.00sec_-14.90C_LIGHT_0190.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20.00sec_-15.00C_LIGHT_0191.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:25.62 -07:39:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7117,14.39,0.05,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 20260118.2117 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-04-Q1b1x1_2025-12-23_00-26-26_20.00sec_-14.90C_LIGHT_0310.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20.00sec_-14.90C_LIGHT_0190.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20.00sec_-15.00C_LIGHT_0191.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:24.54 -07:38:02.7 ;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_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2117 2461058.7117 14.31 06:30:15.50 -07:44:41.5
217.46599 -8.21164 galactic Mon Second-epoch detections are separated by 6.7" 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 | ATO J097.5609-07.7570 | 06:30:16.24 -07:45:18.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.5609-07.7570,2461058.7117,14.31,0.05,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
ATO J097.5609-07.7570 20260118.2117 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-04-Q1b1x1_2025-12-23_00-26-26_20.00sec_-14.90C_LIGHT_0310.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20.00sec_-14.90C_LIGHT_0190.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20.00sec_-15.00C_LIGHT_0191.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:15.50 -07:44:41.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2117 2461058.7117 12.60 05:28:33.94 -15:09:10.1
217.80260 -25.03019 galactic Lep Second-epoch detections are separated by 0.1" 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 2984101946793101312 | 05:28:33.81 -15:09:12.0 (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 2984101946793101312,2461058.7117,12.60,0.05,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 2984101946793101312 20260118.2117 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-04-Q1b1x1_2025-12-23_00-26-26_20.00sec_-14.90C_LIGHT_0310.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-04-Q1b1x1_2025-12-23_00-27-41_20.00sec_-14.90C_LIGHT_0311.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20.00sec_-14.90C_LIGHT_0190.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-04-Q1b1x1_235943_TTUQ1b1x1_18446_gasq95vl/fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20.00sec_-15.00C_LIGHT_0191.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:33.94 -15:09:10.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-05-05_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-17_23-04-12_20_00sec_-14_90C_LIGHT_0190_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2264 2461058.7264 12.81 08:16:52.60 -04:48:48.6
227.44178 16.54372 galactic Hya Second-epoch detections are separated by 3.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J081654.17-044828.9 | 08:16:54.17 -04:48:28.9 (Gaia DR3) | SR (local) | 2458873.59600 (local) | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J081654.17-044828.9,2461058.7264,12.81,0.05,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
ASASSN-V J081654.17-044828.9 20260118.2264 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-05-Q1b1x1_2025-12-23_02-37-17_20.00sec_-14.90C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-05-Q1b1x1_000556_TTUQ1b1x1_3588_L5JV2Eys/fd_Hya-05-Q1b1x1_2026-01-17_23-25-35_20.00sec_-15.00C_LIGHT_0212.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-05-Q1b1x1_000556_TTUQ1b1x1_3588_L5JV2Eys/fd_Hya-05-Q1b1x1_2026-01-17_23-26-13_20.00sec_-14.90C_LIGHT_0213.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:52.60 -04:48:48.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-17_23-26-13_20_00sec_-14_90C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-17_23-25-35_20_00sec_-15_00C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-17_23-26-13_20_00sec_-14_90C_LIGHT_0213_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-17_23-25-35_20_00sec_-15_00C_LIGHT_0212_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.1659* 04 06 49.41 -21 10 29.4 13.6 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
target,2461058.6659,13.56,0.05,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
target 20260118.1659 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Eri-06-Q1b1x1_2025-12-22_21-52-38_20.00sec_-15.00C_LIGHT_0143.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Eri-06-Q1b1x1_001551_TTUQ1b1x1_27159_tJVCwjPP/fd_Eri-06-Q1b1x1_2026-01-17_21-58-18_20.00sec_-14.90C_LIGHT_0124.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Eri-06-Q1b1x1_001551_TTUQ1b1x1_27159_tJVCwjPP/fd_Eri-06-Q1b1x1_2026-01-17_21-59-08_20.00sec_-15.00C_LIGHT_0125.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:06:49.41 -21:10:29.4 ;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_Eri-06-Q1b1x1_2025-12-22_21-52-38_20_00sec_-15_00C_LIGHT_0143_fits__*pix.png resample_wcs_fd_Eri-06-Q1b1x1_2026-01-17_21-59-08_20_00sec_-15_00C_LIGHT_0125_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-06-Q1b1x1_2025-12-22_21-52-38_20_00sec_-15_00C_LIGHT_0143_fits__*pix.png resample_wcs_fd_Eri-06-Q1b1x1_2026-01-17_21-58-18_20_00sec_-14_90C_LIGHT_0124_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-06-Q1b1x1_2025-12-22_21-52-38_20_00sec_-15_00C_LIGHT_0143_fits__*pix.png resample_wcs_fd_Eri-06-Q1b1x1_2026-01-17_21-59-08_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-06-Q1b1x1_2025-12-22_21-52-38_20_00sec_-15_00C_LIGHT_0143_fits__*pix.png resample_wcs_fd_Eri-06-Q1b1x1_2026-01-17_21-58-18_20_00sec_-14_90C_LIGHT_0124_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.1964* 04 58 10.71 -14 15 20.9 13.9 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
target,2461058.6964,13.93,0.05,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 20260118.1964 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lep-01-Q1b1x1_2025-12-22_23-23-57_20.00sec_-15.00C_LIGHT_0236.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lep-01-Q1b1x1_001949_TTUQ1b1x1_26882_w3UvDEGU/fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20.00sec_-15.00C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lep-01-Q1b1x1_001949_TTUQ1b1x1_26882_w3UvDEGU/fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20.00sec_-15.00C_LIGHT_0169.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:10.71 -14:15:20.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20_00sec_-15_00C_LIGHT_0169_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20_00sec_-15_00C_LIGHT_0168_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20_00sec_-15_00C_LIGHT_0169_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20_00sec_-15_00C_LIGHT_0168_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1964 2461058.6964 11.42 04:47:04.75 -20:16:51.9
219.15781 -36.09567 galactic Eri Second-epoch detections are separated by 0.1" 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 | Gaia DR3 2977472029116761344 | 04:47:04.69 -20:16:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.723+/-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 01 18.1964* 04 47 04.75 -20 16 51.9 11.4 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
Gaia DR3 2977472029116761344,2461058.6964,11.42,0.05,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 2977472029116761344 20260118.1964 11.42CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lep-01-Q1b1x1_2025-12-22_23-23-57_20.00sec_-15.00C_LIGHT_0236.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lep-01-Q1b1x1_2025-12-22_23-24-47_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lep-01-Q1b1x1_001949_TTUQ1b1x1_26882_w3UvDEGU/fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20.00sec_-15.00C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lep-01-Q1b1x1_001949_TTUQ1b1x1_26882_w3UvDEGU/fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20.00sec_-15.00C_LIGHT_0169.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:04.75 -20:16:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20_00sec_-15_00C_LIGHT_0169_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20_00sec_-15_00C_LIGHT_0168_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20_00sec_-15_00C_LIGHT_0169_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20_00sec_-15_00C_LIGHT_0168_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1964 2461058.6964 10.52 04:49:01.51 -22:24:22.2
221.83309 -36.34779 galactic Eri Second-epoch detections are separated by 0.2" 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 | Gaia DR3 2973661671570362752 | 04:49:01.54 -22:24:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.655+/-0.041 (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 01 18.1964* 04 49 01.51 -22 24 22.2 10.5 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
Gaia DR3 2973661671570362752,2461058.6964,10.52,0.05,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
Gaia DR3 2973661671570362752 20260118.1964 10.52CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lep-01-Q1b1x1_2025-12-22_23-23-57_20.00sec_-15.00C_LIGHT_0236.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lep-01-Q1b1x1_2025-12-22_23-24-47_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lep-01-Q1b1x1_001949_TTUQ1b1x1_26882_w3UvDEGU/fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20.00sec_-15.00C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lep-01-Q1b1x1_001949_TTUQ1b1x1_26882_w3UvDEGU/fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20.00sec_-15.00C_LIGHT_0169.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:01.51 -22:24:22.2 ;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_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20_00sec_-15_00C_LIGHT_0169_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20_00sec_-15_00C_LIGHT_0168_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-58_20_00sec_-15_00C_LIGHT_0169_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-17_22-42-17_20_00sec_-15_00C_LIGHT_0168_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2224 2461058.7224 14.45 06:23:42.12 +01:03:49.6
208.80791 -5.67930 galactic Mon Second-epoch detections are separated by 5.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.9317+01.0547 | 06:23:44.25 +01:03:32.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.9317+01.0547,2461058.7224,14.45,0.05,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 J095.9317+01.0547 20260118.2224 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ori-06-Q1b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Ori-06-Q1b1x1_233942_TTUQ1b1x1_20346_IbHtnBUn/fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20.00sec_-15.00C_LIGHT_0206.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Ori-06-Q1b1x1_233942_TTUQ1b1x1_20346_IbHtnBUn/fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20.00sec_-14.90C_LIGHT_0207.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:42.12 +01:03:49.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20_00sec_-15_00C_LIGHT_0206_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20_00sec_-14_90C_LIGHT_0207_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20_00sec_-15_00C_LIGHT_0206_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2224 2461058.7224 13.63 05:52:02.69 +00:45:35.4
205.35051 -12.82662 galactic Ori Second-epoch detections are separated by 6.6" 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 3219654750920489728 | 05:52:02.88 +00:45:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1949AnHar.112....1C HD 290908
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.2224* 05 52 02.69 +00 45 35.4 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3219654750920489728,2461058.7224,13.63,0.05,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 3219654750920489728 20260118.2224 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ori-06-Q1b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Ori-06-Q1b1x1_233942_TTUQ1b1x1_20346_IbHtnBUn/fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20.00sec_-15.00C_LIGHT_0206.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Ori-06-Q1b1x1_233942_TTUQ1b1x1_20346_IbHtnBUn/fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20.00sec_-14.90C_LIGHT_0207.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:02.69 +00:45:35.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20_00sec_-15_00C_LIGHT_0206_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20_00sec_-14_90C_LIGHT_0207_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20_00sec_-15_00C_LIGHT_0206_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2224 2461058.7224 14.45 06:21:53.78 -02:49:07.9
212.07737 -7.85623 galactic Mon Second-epoch detections are separated by 1.7" 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 | ATO J095.4701-02.8140 | 06:21:51.62 -02:48:56.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.4701-02.8140,2461058.7224,14.45,0.05,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 J095.4701-02.8140 20260118.2224 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ori-06-Q1b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Ori-06-Q1b1x1_233942_TTUQ1b1x1_20346_IbHtnBUn/fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20.00sec_-15.00C_LIGHT_0206.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Ori-06-Q1b1x1_233942_TTUQ1b1x1_20346_IbHtnBUn/fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20.00sec_-14.90C_LIGHT_0207.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:53.78 -02:49:07.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20_00sec_-15_00C_LIGHT_0206_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-20-33_20_00sec_-14_90C_LIGHT_0207_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-17_23-19-34_20_00sec_-15_00C_LIGHT_0206_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.6009,12.75,0.05,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 20260118.1009 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-02-Q1b1x1_234142_TTUQ1b1x1_30031_39ib5YHn/fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20.00sec_-15.00C_LIGHT_0039.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-02-Q1b1x1_234142_TTUQ1b1x1_30031_39ib5YHn/fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:04:23.74 -04:27:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20_00sec_-15_00C_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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20_00sec_-15_00C_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
target,2461058.6009,13.00,0.05,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
target 20260118.1009 13.00CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-02-Q1b1x1_234142_TTUQ1b1x1_30031_39ib5YHn/fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20.00sec_-15.00C_LIGHT_0039.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-02-Q1b1x1_234142_TTUQ1b1x1_30031_39ib5YHn/fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:16.30 -02:32:53.7 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20_00sec_-15_00C_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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.6009,11.66,0.05,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 20260118.1009 11.66CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-02-Q1b1x1_234142_TTUQ1b1x1_30031_39ib5YHn/fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20.00sec_-15.00C_LIGHT_0039.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Mon-02-Q1b1x1_234142_TTUQ1b1x1_30031_39ib5YHn/fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:27.96 -05:17:19.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20_00sec_-15_00C_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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-25-29_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-17_20-24-44_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 11.49 11:13:24.58 -22:30:17.1
275.03811 35.00221 galactic Crt Second-epoch detections are separated by 3.3" 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 3538101841204005760 | 11:13:25.26 -22:30:25.3 (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 3538101841204005760,2461058.7481,11.49,0.05,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 3538101841204005760 20260118.2481 11.49CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:24.58 -22:30:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 11.47 11:13:06.19 -21:43:12.4
274.52462 35.66947 galactic Crt Second-epoch detections are separated by 1.1" 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 3538961831096367872 | 11:13:06.53 -21:43:16.0 (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 3538961831096367872,2461058.7481,11.47,0.05,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
Gaia DR3 3538961831096367872 20260118.2481 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:06.19 -21:43:12.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 11.56 11:12:58.69 -21:28:16.1
274.35263 35.87770 galactic Crt Second-epoch detections are separated by 1.4" 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 3539355147021105792 | 11:12:59.03 -21:28:19.9 (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 3539355147021105792,2461058.7481,11.56,0.05,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
Gaia DR3 3539355147021105792 20260118.2481 11.56CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:12:58.69 -21:28:16.1 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 11.85 11:13:24.66 -22:02:04.6
274.77844 35.42176 galactic Crt Second-epoch detections are separated by 4.2" 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 | Gaia DR3 3538899777408930944 | 11:13:25.16 -22:02:10.2 (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 3538899777408930944,2461058.7481,11.85,0.05,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
Gaia DR3 3538899777408930944 20260118.2481 11.85CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:24.66 -22:02:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 12.02 11:13:27.64 -22:53:12.7
275.26024 34.66620 galactic Crt Second-epoch detections are separated by 2.7" 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 | Gaia DR3 3538071638994004864 | 11:13:28.50 -22:53:23.0 (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 3538071638994004864,2461058.7481,12.02,0.05,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 3538071638994004864 20260118.2481 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:27.64 -22:53:12.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 12.39 11:13:28.13 -22:23:26.6
274.99021 35.11016 galactic Crt Second-epoch detections are separated by 2.2" 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 3538105071019417216 | 11:13:28.79 -22:23:33.6 (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 3538105071019417216,2461058.7481,12.39,0.05,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
Gaia DR3 3538105071019417216 20260118.2481 12.39CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:28.13 -22:23:26.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 12.64 11:12:58.33 -21:46:57.1
274.52631 35.60005 galactic Crt Second-epoch detections are separated by 0.3" 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 3538959318538675840 | 11:12:58.72 -21:47:00.2 (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 3538959318538675840,2461058.7481,12.64,0.05,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 3538959318538675840 20260118.2481 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:12:58.33 -21:46:57.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 12.81 11:13:28.30 -22:07:09.0
274.84076 35.35273 galactic Crt Second-epoch detections are separated by 2.4" 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 3538887064305730304 | 11:13:28.83 -22:07:14.5 (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 3538887064305730304,2461058.7481,12.81,0.05,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 3538887064305730304 20260118.2481 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:28.30 -22:07:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 12.81 11:12:32.61 -22:59:55.1
275.09235 34.47135 galactic Crt Second-epoch detections are separated by 3.7" 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 3537978249225299840 | 11:12:33.02 -22:59:58.2 (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 3537978249225299840,2461058.7481,12.81,0.05,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 3537978249225299840 20260118.2481 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:12:32.61 -22:59:55.1 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7481,13.12,0.05,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
target 20260118.2481 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:21.00 -22:20:01.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7481,13.39,0.05,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 20260118.2481 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:29.01 -22:26:28.0 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 11.74 11:09:40.81 -22:10:21.5
273.91725 34.90200 galactic Crt 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 | ATO J167.4201-22.1726 | 11:09:40.84 -22:10:21.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.487+/-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
ATO J167.4201-22.1726,2461058.7481,11.74,0.05,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
ATO J167.4201-22.1726 20260118.2481 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:09:40.81 -22:10:21.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 10.80 11:03:50.11 -21:00:22.6
271.77647 35.27352 galactic Crt Second-epoch detections are separated by 0.5" 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 | Gaia DR3 3551220492391592704 | 11:03:50.17 -21:00:22.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.322+/-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 3551220492391592704,2461058.7481,10.80,0.05,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
Gaia DR3 3551220492391592704 20260118.2481 10.80CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:50.11 -21:00:22.6 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 12.44 11:06:34.83 -21:14:10.9
272.59910 35.38492 galactic Crt Second-epoch detections are separated by 2.1" 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 | ATO J166.6432-21.2359 | 11:06:34.94 -21:14:11.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J166.6432-21.2359,2461058.7481,12.44,0.05,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
ATO J166.6432-21.2359 20260118.2481 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:06:34.83 -21:14:10.9 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 10.54 11:04:45.75 -22:58:59.7
273.17089 33.65085 galactic Crt Second-epoch detections are separated by 0.6" 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 3537449418491653632 | 11:04:45.73 -22:58:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.112+/-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 3537449418491653632,2461058.7481,10.54,0.05,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 3537449418491653632 20260118.2481 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:04:45.75 -22:58:59.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2481 2461058.7481 12.30 11:00:34.47 -21:27:29.4
271.24727 34.50338 galactic Crt Second-epoch detections are separated by 0.3" 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 | Gaia DR3 3549867852571411072 | 11:00:34.53 -21:27:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.789+/-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 3549867852571411072,2461058.7481,12.30,0.05,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 3549867852571411072 20260118.2481 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-56-37_20.00sec_-14.90C_LIGHT_0243.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-09-Q1b1x1_003316_TTUQ1b1x1_9576_zqggqyYq/fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20.00sec_-14.90C_LIGHT_0244.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:00:34.47 -21:27:29.4 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_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_2026-01-17_23-57-37_20_00sec_-14_90C_LIGHT_0244_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_2026-01-17_23-56-37_20_00sec_-14_90C_LIGHT_0243_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2209 2461058.7209 10.18 10:09:37.04 -30:55:47.7
266.53691 20.27540 galactic Ant Second-epoch detections are separated by 2.4" 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 5460323766019112192 | 10:09:38.19 -30:56:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0III 1982MSS...C03....0H HD 88200
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 01 18.2209* 10 09 37.04 -30 55 47.7 10.2 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
Gaia DR3 5460323766019112192,2461058.7209,10.18,0.05,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
Gaia DR3 5460323766019112192 20260118.2209 10.18CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20.00sec_-14.90C_LIGHT_0204.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20.00sec_-14.90C_LIGHT_0205.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:37.04 -30:55:47.7 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2209 2461058.7209 10.44 10:12:07.83 -30:54:20.4
266.97587 20.62464 galactic Ant Second-epoch detections are separated by 2.9" 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 5461813157597324288 | 10:12:09.52 -30:54:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8IV/V 1982MSS...C03....0H HD 88553
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 01 18.2209* 10 12 07.83 -30 54 20.4 10.4 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
Gaia DR3 5461813157597324288,2461058.7209,10.44,0.05,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 5461813157597324288 20260118.2209 10.44CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20.00sec_-14.90C_LIGHT_0204.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20.00sec_-14.90C_LIGHT_0205.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:12:07.83 -30:54:20.4 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2209 2461058.7209 10.85 10:09:22.92 -30:55:29.6
266.49123 20.24828 galactic Ant Second-epoch detections are separated by 2.7" 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 5460323662939895808 | 10:09:24.03 -30:55:43.7 (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 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 01 18.2209* 10 09 22.92 -30 55 29.6 10.8 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
Gaia DR3 5460323662939895808,2461058.7209,10.85,0.05,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
Gaia DR3 5460323662939895808 20260118.2209 10.85CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20.00sec_-14.90C_LIGHT_0204.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20.00sec_-14.90C_LIGHT_0205.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:22.92 -30:55:29.6 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2209 2461058.7209 11.01 10:06:51.23 -31:05:43.0
266.15086 19.77903 galactic Ant Second-epoch detections are separated by 0.3" 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 | Gaia DR3 5460493193888524800 | 10:06:51.91 -31:05:51.7 (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 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 01 18.2209* 10 06 51.23 -31 05 43.0 11.0 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
Gaia DR3 5460493193888524800,2461058.7209,11.01,0.05,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
Gaia DR3 5460493193888524800 20260118.2209 11.01CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20.00sec_-14.90C_LIGHT_0204.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20.00sec_-14.90C_LIGHT_0205.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:06:51.23 -31:05:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2209 2461058.7209 11.19 10:07:40.94 -30:58:53.0
266.22346 19.97854 galactic Ant Second-epoch detections are separated by 0.3" 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 | Gaia DR3 5460500753030988672 | 10:07:40.43 -30:58:46.0 (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 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 01 18.2209* 10 07 40.94 -30 58 53.0 11.2 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
Gaia DR3 5460500753030988672,2461058.7209,11.19,0.05,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 5460500753030988672 20260118.2209 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20.00sec_-14.90C_LIGHT_0204.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20.00sec_-14.90C_LIGHT_0205.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:07:40.94 -30:58:53.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2209 2461058.7209 11.39 10:10:56.83 -30:58:38.8
266.80808 20.41288 galactic Ant Second-epoch detections are separated by 1.9" 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 5460313767336112128 | 10:10:58.27 -30:58:56.6 (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 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 01 18.2209* 10 10 56.83 -30 58 38.8 11.4 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
Gaia DR3 5460313767336112128,2461058.7209,11.39,0.05,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
Gaia DR3 5460313767336112128 20260118.2209 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20.00sec_-14.90C_LIGHT_0204.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20.00sec_-14.90C_LIGHT_0205.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:10:56.83 -30:58:38.8 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2209 2461058.7209 10.23 10:03:29.45 -30:56:21.2
265.45104 19.44893 galactic Ant Second-epoch detections are separated by 1.4" 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 | Gaia DR3 5463465483055780352 | 10:03:29.49 -30:56:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.950+/-0.044 (M)
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 01 18.2209* 10 03 29.45 -30 56 21.2 10.2 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
Gaia DR3 5463465483055780352,2461058.7209,10.23,0.05,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
Gaia DR3 5463465483055780352 20260118.2209 10.23CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-01-Q1b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20.00sec_-14.90C_LIGHT_0204.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-01-Q1b1x1_004651_TTUQ1b1x1_19982_wiLNMIet/fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20.00sec_-14.90C_LIGHT_0205.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:03:29.45 -30:56:21.2 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-18-17_20_00sec_-14_90C_LIGHT_0205_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-17_23-17-33_20_00sec_-14_90C_LIGHT_0204_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.86 07:22:50.00 -14:06:33.3
229.03408 0.38473 galactic CMa Second-epoch detections are separated by 0.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:22:50.00 -14:06:33.3 (user input) | T | P | (position from user input) J-Ks=0.225+/-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
target,2461058.5913,12.86,0.05,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
target 20260118.0913 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:22:50.00 -14:06:33.3 ;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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.43 07:23:11.75 -14:56:19.1
229.80665 0.07053 galactic CMa 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 | ATO J110.8075-14.9328 | 07:23:11.80 -14:56:18.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.692+/-0.029 (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
ATO J110.8075-14.9328,2461058.5913,12.43,0.05,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
ATO J110.8075-14.9328 20260118.0913 12.43CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:23:11.75 -14:56:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 11.28 07:23:00.93 -14:56:29.4
229.78861 0.03079 galactic CMa Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3031585902635038208 | 07:23:00.95 -14:56:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.687+/-0.035 (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 3031585902635038208,2461058.5913,11.28,0.05,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
Gaia DR3 3031585902635038208 20260118.0913 11.28CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:23:00.93 -14:56:29.4 ;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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 10.18 07:21:57.19 -14:46:12.0
229.51632 -0.11471 galactic CMa Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3031781856222010368 | 07:21:57.24 -14:46:10.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.123+/-0.032 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 3031781856222010368,2461058.5913,10.18,0.05,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
Gaia DR3 3031781856222010368 20260118.0913 10.18CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:21:57.19 -14:46:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 11.07 07:23:12.75 -14:36:13.8
229.51344 0.23220 galactic CMa Second-epoch detections are separated by 0.8" 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 3031806285997148416 | 07:23:12.77 -14:36:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.708+/-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 3031806285997148416,2461058.5913,11.07,0.05,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
Gaia DR3 3031806285997148416 20260118.0913 11.07CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:23:12.75 -14:36:13.8 ;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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.68 07:20:47.57 -14:00:04.0
228.70565 -0.00090 galactic CMa Second-epoch detections are separated by 1.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J110.1989-13.9981 | 07:20:47.62 -14:00:04.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.328+/-0.031 (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 J110.1989-13.9981,2461058.5913,12.68,0.05,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
ATO J110.1989-13.9981 20260118.0913 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:20:47.57 -14:00:04.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.63 07:19:54.10 -15:03:38.7
229.54001 -0.68881 galactic CMa Second-epoch detections are separated by 1.1" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3031401528278884480 | 07:19:54.18 -15:03:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.770+/-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
Gaia DR3 3031401528278884480,2461058.5913,12.63,0.05,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 3031401528278884480 20260118.0913 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:19:54.10 -15:03:38.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.68 07:21:59.16 -14:57:15.7
229.68269 -0.19456 galactic CMa Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | TT CMa | 07:22:01.97 -14:56:57.0 (Gaia DR3) | M (local) | 2453078.00000 (local) | Gaia3var=VARIABLE SpType: S 1956ApJ...124..346C TT CMa J-Ks=0.142+/-0.030 (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
TT CMa,2461058.5913,12.68,0.05,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
TT CMa 20260118.0913 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:21:59.16 -14:57:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.36 07:22:22.29 -13:50:19.7
228.74275 0.41348 galactic CMa Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J110.5911-13.8435 | 07:22:22.37 -13:50:19.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.146+/-0.033 (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
ATO J110.5911-13.8435,2461058.5913,12.36,0.05,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
ATO J110.5911-13.8435 20260118.0913 12.36CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:22:22.29 -13:50:19.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.63 07:22:53.86 -14:49:55.8
229.67878 0.05730 galactic CMa Second-epoch detections are separated by 1.1" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J110.7372-14.8353 | 07:22:53.88 -14:49:54.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-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 J110.7372-14.8353,2461058.5913,12.63,0.05,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
ATO J110.7372-14.8353 20260118.0913 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:22:53.86 -14:49:55.8 ;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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.25 07:22:26.88 -15:05:53.6
229.86214 -0.16397 galactic CMa Second-epoch detections are separated by 1.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3031576866024036736 | 07:22:26.91 -15:05:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.078+/-0.035 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 3031576866024036736,2461058.5913,12.25,0.05,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
Gaia DR3 3031576866024036736 20260118.0913 12.25CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:22:26.88 -15:05:53.6 ;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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 12.77 07:19:25.56 -14:50:11.7
229.28813 -0.68521 galactic CMa Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3031460833189177088 | 07:19:23.84 -14:50:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.748+/-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 3031460833189177088,2461058.5913,12.77,0.05,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
Gaia DR3 3031460833189177088 20260118.0913 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:19:25.56 -14:50:11.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.0913 2461058.5913 11.80 07:23:58.46 -14:41:50.3
229.68291 0.35041 galactic CMa Second-epoch detections are separated by 1.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3031621911642625152 | 07:23:58.69 -14:41:52.9 (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 3031621911642625152,2461058.5913,11.80,0.05,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
Gaia DR3 3031621911642625152 20260118.0913 11.80CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20.00sec_-14.90C_LIGHT_0023.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-05-Q1b1x1_000218_TTUQ1b1x1_13343_WRbWDXeA/fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:23:58.46 -14:41:50.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-40_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-17_20-11-04_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1631 2461058.6631 14.34 00:37:21.54 +42:00:59.0
120.13565 -20.77891 galactic And Second-epoch detections are separated by 3.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 varaible 381465289991471104 | 00:37:21.54 +42:00:59.0 (user input) | | 2022yCat.1358....0G | (position from user input) Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') J-Ks=0.713+/-0.062 (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 01 18.1631* 00 37 21.54 +42 00 59.0 14.3 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 varaible 381465289991471104,2461058.6631,14.34,0.05,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 varaible 381465289991471104 20260118.1631 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 /mnt/usb2/NMW-TexasTech/reference_imgs/And-04-Q1b1x1_2025-12-22_21-39-44_20.00sec_-15.00C_LIGHT_0127.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_And-04-Q1b1x1_221536_TTUQ1b1x1_28549_2D4JNnWz/fd_And-04-Q1b1x1_2026-01-17_21-54-23_20.00sec_-14.90C_LIGHT_0120.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_And-04-Q1b1x1_221536_TTUQ1b1x1_28549_2D4JNnWz/fd_And-04-Q1b1x1_2026-01-17_21-55-03_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:21.54 +42:00:59.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-17_21-55-03_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-17_21-54-23_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_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-17_21-55-03_20_00sec_-15_00C_LIGHT_0121_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-17_21-54-23_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 01 18.1631* 23 43 23.88 +43 09 03.7 13.7 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,2461058.6631,13.68,0.05,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
target 20260118.1631 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/And-04-Q1b1x1_2025-12-22_21-39-44_20.00sec_-15.00C_LIGHT_0127.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_And-04-Q1b1x1_221536_TTUQ1b1x1_28549_2D4JNnWz/fd_And-04-Q1b1x1_2026-01-17_21-54-23_20.00sec_-14.90C_LIGHT_0120.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_And-04-Q1b1x1_221536_TTUQ1b1x1_28549_2D4JNnWz/fd_And-04-Q1b1x1_2026-01-17_21-55-03_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:43:23.88 +43:09:03.7 ;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_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-17_21-55-03_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-17_21-54-23_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_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-17_21-55-03_20_00sec_-15_00C_LIGHT_0121_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-17_21-54-23_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 10.70 11:05:33.44 -38:52:52.0
281.33258 19.50917 galactic Ant Second-epoch detections are separated by 4.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5396793125172481280 | 11:05:34.93 -38:53:09.8 (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 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 01 18.2876* 11 05 33.44 -38 52 52.0 10.7 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
Gaia DR3 5396793125172481280,2461058.7877,10.70,0.05,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 5396793125172481280 20260118.2877 10.70CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:33.44 -38:52:52.0 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 10.66 11:01:15.31 -39:00:38.6
280.59054 19.03390 galactic Ant Second-epoch detections are separated by 3.9" 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 | Gaia DR3 5393779398160751104 | 11:01:16.15 -39:00:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 01 18.2876* 11 01 15.31 -39 00 38.6 10.7 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
Gaia DR3 5393779398160751104,2461058.7877,10.66,0.05,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 5393779398160751104 20260118.2877 10.66CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:01:15.31 -39:00:38.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 10.79 11:04:32.73 -38:35:09.9
281.01031 19.69304 galactic Ant Second-epoch detections are separated by 7.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5396815149765767936 | 11:04:33.67 -38:35:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1955AnCap..18.....J CD-37 7016
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 01 18.2876* 11 04 32.73 -38 35 09.9 10.8 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
Gaia DR3 5396815149765767936,2461058.7877,10.79,0.05,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
Gaia DR3 5396815149765767936 20260118.2877 10.79CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:04:32.73 -38:35:09.9 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 10.96 11:02:44.60 -38:44:55.8
280.74686 19.39540 galactic Ant Second-epoch detections are separated by 4.2" 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 | Gaia DR3 5393812658387533568 | 11:02:45.45 -38:45:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 01 18.2876* 11 02 44.60 -38 44 55.8 11.0 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
Gaia DR3 5393812658387533568,2461058.7877,10.96,0.05,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
Gaia DR3 5393812658387533568 20260118.2877 10.96CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:02:44.60 -38:44:55.8 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 10.13 11:03:30.07 -39:01:07.6
281.01078 19.21490 galactic Ant Second-epoch detections are separated by 5.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5390795186164872448 | 11:03:31.24 -39:01:22.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 1955AnCap..18.....J CD-38 6904
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 01 18.2876* 11 03 30.07 -39 01 07.6 10.1 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
Gaia DR3 5390795186164872448,2461058.7877,10.13,0.05,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 5390795186164872448 20260118.2877 10.13CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-48_20.00sec_-14.90C_LIGHT_0015.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:30.07 -39:01:07.6 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 10.60 11:02:45.08 -38:45:02.1
280.74915 19.39449 galactic Ant Second-epoch detections are separated by 2.1" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5393812658387533568 | 11:02:45.45 -38:45:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 01 18.2876* 11 02 45.08 -38 45 02.1 10.6 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
Gaia DR3 5393812658387533568,2461058.7877,10.60,0.05,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 5393812658387533568 20260118.2877 10.60CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:02:45.08 -38:45:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.18 11:04:44.42 -37:53:41.8
280.73412 20.33475 galactic Ant Second-epoch detections are separated by 8.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5399872651083986688 | 11:04:44.80 -37:53:46.5 (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 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 01 18.2876* 11 04 44.42 -37 53 41.8 11.2 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
Gaia DR3 5399872651083986688,2461058.7877,11.18,0.05,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
Gaia DR3 5399872651083986688 20260118.2877 11.18CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:04:44.42 -37:53:41.8 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.18 10:58:37.84 -39:02:10.7
280.11854 18.78673 galactic Ant Second-epoch detections are separated by 0.5" and 6.1 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 5393743286075574656 | 10:58:38.48 -39:02:19.0 (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 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 01 18.2876* 10 58 37.84 -39 02 10.7 11.2 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
Gaia DR3 5393743286075574656,2461058.7877,11.18,0.05,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
Gaia DR3 5393743286075574656 20260118.2877 11.18CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:58:37.84 -39:02:10.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.32 11:03:13.96 -38:39:51.8
280.79973 19.51269 galactic Ant Second-epoch detections are separated by 1.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5393811936833103744 | 11:03:14.44 -38:39:57.6 (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 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 01 18.2876* 11 03 13.96 -38 39 51.8 11.3 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
Gaia DR3 5393811936833103744,2461058.7877,11.32,0.05,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
Gaia DR3 5393811936833103744 20260118.2877 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:13.96 -38:39:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.14 11:03:42.83 -39:00:40.4
281.04691 19.23938 galactic Ant Second-epoch detections are separated by 4.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5390800271405007488 | 11:03:44.07 -39:00:55.7 (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 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 01 18.2876* 11 03 42.83 -39 00 40.4 11.1 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
Gaia DR3 5390800271405007488,2461058.7877,11.14,0.05,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 5390800271405007488 20260118.2877 11.14CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:42.83 -39:00:40.4 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.29 11:04:49.92 -38:53:39.6
281.20278 19.43760 galactic Ant Second-epoch detections are separated by 2.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5396794946238599680 | 11:04:51.21 -38:53:56.4 (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!
TCP 2026 01 18.2876* 11 04 49.92 -38 53 39.6 11.3 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
Gaia DR3 5396794946238599680,2461058.7877,11.29,0.05,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 5396794946238599680 20260118.2877 11.29CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:04:49.92 -38:53:39.6 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.62 11:03:50.32 -38:10:22.5
280.68965 20.00757 galactic Ant Second-epoch detections are separated by 7.6" 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 | Gaia DR3 5399844132498785024 | 11:03:50.77 -38:10:27.9 (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 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 01 18.2876* 11 03 50.32 -38 10 22.5 11.6 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
Gaia DR3 5399844132498785024,2461058.7877,11.62,0.05,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
Gaia DR3 5399844132498785024 20260118.2877 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:50.32 -38:10:22.5 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.72 11:03:54.60 -38:19:03.9
280.76909 19.88268 galactic Ant Second-epoch detections are separated by 5.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5399830354246000640 | 11:03:55.00 -38:19:08.1 (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!
TCP 2026 01 18.2876* 11 03 54.60 -38 19 03.9 11.7 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
Gaia DR3 5399830354246000640,2461058.7877,11.72,0.05,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 5399830354246000640 20260118.2877 11.72CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:54.60 -38:19:03.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.71 11:01:42.82 -38:46:56.6
280.57047 19.27831 galactic Ant Second-epoch detections are separated by 6.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5393817846708011648 | 11:01:43.11 -38:47:01.5 (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 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 01 18.2876* 11 01 42.82 -38 46 56.6 11.7 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
Gaia DR3 5393817846708011648,2461058.7877,11.71,0.05,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
Gaia DR3 5393817846708011648 20260118.2877 11.71CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:01:42.82 -38:46:56.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.71 11:03:22.66 -38:59:18.4
280.97407 19.23205 galactic Ant Second-epoch detections are separated by 5.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5390795495401371776 | 11:03:23.75 -38:59:34.3 (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!
TCP 2026 01 18.2876* 11 03 22.66 -38 59 18.4 11.7 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
Gaia DR3 5390795495401371776,2461058.7877,11.71,0.05,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
Gaia DR3 5390795495401371776 20260118.2877 11.71CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:22.66 -38:59:18.4 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.91 11:04:45.89 -38:46:19.6
281.13529 19.54278 galactic Ant Second-epoch detections are separated by 4.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5396808415255903872 | 11:04:47.06 -38:46:34.9 (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 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 01 18.2876* 11 04 45.89 -38 46 19.6 11.9 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
Gaia DR3 5396808415255903872,2461058.7877,11.91,0.05,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 5396808415255903872 20260118.2877 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:04:45.89 -38:46:19.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 11.88 11:04:20.93 -38:45:56.2
281.05446 19.51423 galactic Ant Second-epoch detections are separated by 4.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5396809033732332288 | 11:04:22.04 -38:46:10.4 (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!
TCP 2026 01 18.2876* 11 04 20.93 -38 45 56.2 11.9 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
Gaia DR3 5396809033732332288,2461058.7877,11.88,0.05,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
Gaia DR3 5396809033732332288 20260118.2877 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:04:20.93 -38:45:56.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 12.15 11:02:13.35 -38:45:37.9
280.65513 19.34101 galactic Ant Second-epoch detections are separated by 6.3" 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 | Gaia DR3 5393807366987818368 | 11:02:13.63 -38:45:42.8 (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 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 01 18.2876* 11 02 13.35 -38 45 37.9 12.2 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
Gaia DR3 5393807366987818368,2461058.7877,12.15,0.05,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
Gaia DR3 5393807366987818368 20260118.2877 12.15CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:02:13.35 -38:45:37.9 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2877 2461058.7877 12.09 11:02:12.93 -38:50:27.0
280.69063 19.26801 galactic Ant Second-epoch detections are separated by 1.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5393804824367169536 | 11:02:13.25 -38:50:32.1 (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!
TCP 2026 01 18.2876* 11 02 12.93 -38 50 27.0 12.1 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
Gaia DR3 5393804824367169536,2461058.7877,12.09,0.05,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
Gaia DR3 5393804824367169536 20260118.2877 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20.00sec_-15.00C_LIGHT_0282.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ant-02-Q1b1x1_010250_TTUQ1b1x1_16628_Awl85ms7/fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20.00sec_-14.90C_LIGHT_0283.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:02:12.93 -38:50:27.0 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-54-29_20_00sec_-14_90C_LIGHT_0283_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-18_00-53-36_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3039 2461058.8039 13.39 07:45:53.26 +57:11:45.1
160.28305 29.78499 galactic Lyn Second-epoch detections are separated by 0.7" 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 J116.4721+57.1957 | 07:45:53.26 +57:11:45.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.316+/-0.031 (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 J116.4721+57.1957,2461058.8039,13.39,0.05,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
ATO J116.4721+57.1957 20260118.3039 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2025-12-23_04-26-38_20.00sec_-15.00C_LIGHT_0554.fits /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2025-12-23_04-27-26_20.00sec_-15.00C_LIGHT_0555.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_UMa-02-Q1b1x1_014430_TTUQ1b1x1_20971_lhEgpx0j/fd_UMa-02-Q1b1x1_2026-01-18_01-16-52_20.00sec_-15.00C_LIGHT_0304.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_UMa-02-Q1b1x1_014430_TTUQ1b1x1_20971_lhEgpx0j/fd_UMa-02-Q1b1x1_2026-01-18_01-17-53_20.00sec_-15.00C_LIGHT_0305.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:53.26 +57:11:45.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-02-Q1b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q1b1x1_2026-01-18_01-17-53_20_00sec_-15_00C_LIGHT_0305_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-02-Q1b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q1b1x1_2026-01-18_01-16-52_20_00sec_-15_00C_LIGHT_0304_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-02-Q1b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q1b1x1_2026-01-18_01-17-53_20_00sec_-15_00C_LIGHT_0305_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-02-Q1b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q1b1x1_2026-01-18_01-16-52_20_00sec_-15_00C_LIGHT_0304_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1474 2461058.6474 13.99 22:12:39.38 +50:21:42.1
98.79236 -4.91713 galactic Lac Second-epoch detections are separated by 8.5" and 3.5 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 J333.1633+50.3635 | 22:12:39.38 +50:21:42.1 (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 J333.1633+50.3635,2461058.6474,13.99,0.05,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 J333.1633+50.3635 20260118.1474 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lac-02-Q1b1x1_2025-12-22_21-14-54_20.00sec_-15.00C_LIGHT_0094.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Lac-02-Q1b1x1_221333_TTUQ1b1x1_27092_0h6NagN7/fd_Lac-02-Q1b1x1_2026-01-17_21-31-37_20.00sec_-15.00C_LIGHT_0100.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Lac-02-Q1b1x1_221333_TTUQ1b1x1_27092_0h6NagN7/fd_Lac-02-Q1b1x1_2026-01-17_21-32-31_20.00sec_-15.00C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:39.38 +50:21:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lac-02-Q1b1x1_2025-12-22_21-14-54_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png resample_wcs_fd_Lac-02-Q1b1x1_2026-01-17_21-32-31_20_00sec_-15_00C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-02-Q1b1x1_2025-12-22_21-14-54_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png resample_wcs_fd_Lac-02-Q1b1x1_2026-01-17_21-31-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-02-Q1b1x1_2025-12-22_21-14-54_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png resample_wcs_fd_Lac-02-Q1b1x1_2026-01-17_21-32-31_20_00sec_-15_00C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-02-Q1b1x1_2025-12-22_21-14-54_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png resample_wcs_fd_Lac-02-Q1b1x1_2026-01-17_21-31-37_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7989,13.43,0.05,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
target 20260118.2989 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-05-Q1b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-05-Q1b1x1_013641_TTUQ1b1x1_27959_85JlEQVV/fd_Dra-05-Q1b1x1_2026-01-18_01-09-46_20.00sec_-14.90C_LIGHT_0298.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-05-Q1b1x1_013641_TTUQ1b1x1_27959_85JlEQVV/fd_Dra-05-Q1b1x1_2026-01-18_01-10-36_20.00sec_-15.00C_LIGHT_0299.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:50.36 +65:20:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q1b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q1b1x1_2026-01-18_01-10-36_20_00sec_-15_00C_LIGHT_0299_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_2026-01-18_01-09-46_20_00sec_-14_90C_LIGHT_0298_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_2026-01-18_01-10-36_20_00sec_-15_00C_LIGHT_0299_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_2026-01-18_01-09-46_20_00sec_-14_90C_LIGHT_0298_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2989 2461058.7989 10.79 18:22:42.13 +63:21:01.6
92.90237 27.22356 galactic Dra Second-epoch detections are separated by 2.1" and 3.5 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 J275.6643+63.3604 | 18:22:42.26 +63:21:00.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.226+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J275.6643+63.3604,2461058.7989,10.79,0.05,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
ATO J275.6643+63.3604 20260118.2989 10.79CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-05-Q1b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-05-Q1b1x1_2026-01-09_02-58-25_20.00sec_-15.00C_LIGHT_0033.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-05-Q1b1x1_013641_TTUQ1b1x1_27959_85JlEQVV/fd_Dra-05-Q1b1x1_2026-01-18_01-09-46_20.00sec_-14.90C_LIGHT_0298.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-05-Q1b1x1_013641_TTUQ1b1x1_27959_85JlEQVV/fd_Dra-05-Q1b1x1_2026-01-18_01-10-36_20.00sec_-15.00C_LIGHT_0299.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:22:42.13 +63:21:01.6 ;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_Dra-05-Q1b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q1b1x1_2026-01-18_01-10-36_20_00sec_-15_00C_LIGHT_0299_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_2026-01-18_01-09-46_20_00sec_-14_90C_LIGHT_0298_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_2026-01-18_01-10-36_20_00sec_-15_00C_LIGHT_0299_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_2026-01-18_01-09-46_20_00sec_-14_90C_LIGHT_0298_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.13,0.05,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
target 20260118.2894 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:02:48.32 +71:44:53.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,12.36,0.05,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
target 20260118.2894 12.36CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:30.54 +68:51:25.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2894 2461058.7894 12.78 03:47:34.98 +71:40:32.6
135.91445 13.39767 galactic Cam Second-epoch detections are separated by 8.8" 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 543297012007204864 | 03:47:37.62 +71:41:13.3 (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 543297012007204864,2461058.7894,12.78,0.05,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
Gaia DR3 543297012007204864 20260118.2894 12.78CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:34.98 +71:40:32.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.26,0.05,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 20260118.2894 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:06.16 +72:32:46.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2894 2461058.7894 13.26 03:36:38.51 +74:56:35.9
133.17913 15.46458 galactic Cas Second-epoch detections are separated by 4.3" 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 544914187452032512 | 03:36:30.76 +74:56:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.2894* 03 36 38.51 +74 56 35.9 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 544914187452032512,2461058.7894,13.26,0.05,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
Gaia DR3 544914187452032512 20260118.2894 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:38.51 +74:56:35.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.28,0.05,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
target 20260118.2894 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:54.44 +72:20:28.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2894 2461058.7894 13.48 03:43:14.78 +71:23:46.9
135.82084 12.96451 galactic Cam Second-epoch detections are separated by 6.1" 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 543274162780514944 | 03:43:10.57 +71:24:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.608+/-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 543274162780514944,2461058.7894,13.48,0.05,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
Gaia DR3 543274162780514944 20260118.2894 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:14.78 +71:23:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.37,0.05,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 20260118.2894 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:47.95 +68:14:07.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.56,0.05,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
target 20260118.2894 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:24.05 +70:57:48.7 ;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-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.63,0.05,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
target 20260118.2894 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:52.28 +66:22:18.1 ;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-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.55,0.05,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
target 20260118.2894 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:44.05 +74:39:46.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.62,0.05,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 20260118.2894 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:43.31 +73:29:22.9 ;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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.57,0.05,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 20260118.2894 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:58.76 +69:47:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7894,13.71,0.05,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
target 20260118.2894 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:56.57 +68:24:20.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.2894* 03 38 03.79 +73 10 58.8 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,2461058.7894,13.55,0.05,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
target 20260118.2894 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-56-10_20.00sec_-15.00C_LIGHT_0284.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-06-Q1b1x1_012446_TTUQ1b1x1_8227_dZsPIzGa/fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20.00sec_-15.00C_LIGHT_0285.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:03.79 +73:10:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_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_2026-01-18_00-57-04_20_00sec_-15_00C_LIGHT_0285_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_2026-01-18_00-56-10_20_00sec_-15_00C_LIGHT_0284_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3106 2461058.8106 9.83 18:06:52.23 +57:45:31.5
86.36899 28.51731 galactic Dra Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2152030579553827200 | 18:06:51.51 +57:45:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1928AnHar.100...49C HD 238814
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 2152030579553827200,2461058.8106,9.83,0.05,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
Gaia DR3 2152030579553827200 20260118.3106 9.83CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-07-Q1b1x1_2025-12-23_06-37-17_20.00sec_-15.00C_LIGHT_0702.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-07-Q1b1x1_015514_TTUQ1b1x1_13612_qB7IsfIc/fd_Dra-07-Q1b1x1_2026-01-18_01-26-36_20.00sec_-15.00C_LIGHT_0314.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-07-Q1b1x1_015514_TTUQ1b1x1_13612_qB7IsfIc/fd_Dra-07-Q1b1x1_2026-01-18_01-27-26_20.00sec_-14.90C_LIGHT_0315.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:06:52.23 +57:45:31.5 ;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_Dra-07-Q1b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q1b1x1_2026-01-18_01-27-26_20_00sec_-14_90C_LIGHT_0315_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_2026-01-18_01-26-36_20_00sec_-15_00C_LIGHT_0314_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_2026-01-18_01-27-26_20_00sec_-14_90C_LIGHT_0315_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_2026-01-18_01-26-36_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3106 2461058.8106 11.81 18:10:17.54 +57:27:00.2
86.08277 28.02558 galactic Dra Second-epoch detections are separated by 1.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2151821019510500096 | 18:10:16.81 +57:27:04.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2151821019510500096,2461058.8106,11.81,0.05,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 2151821019510500096 20260118.3106 11.81CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-07-Q1b1x1_2025-12-23_06-37-17_20.00sec_-15.00C_LIGHT_0702.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-07-Q1b1x1_015514_TTUQ1b1x1_13612_qB7IsfIc/fd_Dra-07-Q1b1x1_2026-01-18_01-26-36_20.00sec_-15.00C_LIGHT_0314.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-07-Q1b1x1_015514_TTUQ1b1x1_13612_qB7IsfIc/fd_Dra-07-Q1b1x1_2026-01-18_01-27-26_20.00sec_-14.90C_LIGHT_0315.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:10:17.54 +57:27:00.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-07-Q1b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q1b1x1_2026-01-18_01-27-26_20_00sec_-14_90C_LIGHT_0315_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_2026-01-18_01-26-36_20_00sec_-15_00C_LIGHT_0314_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_2026-01-18_01-27-26_20_00sec_-14_90C_LIGHT_0315_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_2026-01-18_01-26-36_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1437 2461058.6437 13.96 22:39:34.63 +37:45:39.6
96.01918 -18.12497 galactic Lac Second-epoch detections are separated by 0.5" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J339.8946+37.7632 | 22:39:34.63 +37:45:39.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J339.8946+37.7632,2461058.6437,13.96,0.05,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
ATO J339.8946+37.7632 20260118.1437 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lac-03-Q1b1x1_2025-12-22_21-04-39_20.00sec_-14.90C_LIGHT_0086.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Lac-03-Q1b1x1_222529_TTUQ1b1x1_13118_ZqxIkGCx/fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20.00sec_-14.90C_LIGHT_0094.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Lac-03-Q1b1x1_222529_TTUQ1b1x1_13118_ZqxIkGCx/fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:39:34.63 +37:45:39.6 ;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_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1437 2461058.6437 12.71 22:18:04.37 +32:46:23.7
89.24457 -19.88284 galactic Peg Second-epoch detections are separated by 1.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J334.5206+32.7699 | 22:18:04.30 +32:46:23.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.588+/-0.029 (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
ATO J334.5206+32.7699,2461058.6437,12.71,0.05,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
ATO J334.5206+32.7699 20260118.1437 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lac-03-Q1b1x1_2025-12-22_21-04-39_20.00sec_-14.90C_LIGHT_0086.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lac-03-Q1b1x1_2025-12-22_21-05-25_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Lac-03-Q1b1x1_222529_TTUQ1b1x1_13118_ZqxIkGCx/fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20.00sec_-14.90C_LIGHT_0094.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Lac-03-Q1b1x1_222529_TTUQ1b1x1_13118_ZqxIkGCx/fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:04.37 +32:46:23.7 ;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_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1437 2461058.6437 12.96 22:21:42.29 +33:18:41.8
90.23596 -19.88713 galactic Peg Second-epoch detections are separated by 1.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:21:42.29 +33:18:41.8 (user input) | T | P | (position from user input) J-Ks=0.603+/-0.027 (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,2461058.6437,12.96,0.05,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
target 20260118.1437 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lac-03-Q1b1x1_2025-12-22_21-04-39_20.00sec_-14.90C_LIGHT_0086.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lac-03-Q1b1x1_2025-12-22_21-05-25_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Lac-03-Q1b1x1_222529_TTUQ1b1x1_13118_ZqxIkGCx/fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20.00sec_-14.90C_LIGHT_0094.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Lac-03-Q1b1x1_222529_TTUQ1b1x1_13118_ZqxIkGCx/fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:42.29 +33:18:41.8 ;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_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-27-01_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lac-03-Q1b1x1_2025-12-22_21-04-39_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png resample_wcs_fd_Lac-03-Q1b1x1_2026-01-17_21-26-23_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2467 2461058.7467 14.03 05:25:32.60 +63:26:27.8
148.47352 15.20032 galactic Cam Second-epoch detections are separated by 6.1" 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 | Gaia DR3 287443645520212736 | 05:25:34.54 +63:26:08.3 (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 287443645520212736,2461058.7467,14.03,0.05,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
Gaia DR3 287443645520212736 20260118.2467 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2025-12-23_02-00-56_20.00sec_-15.00C_LIGHT_0407.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-09-Q1b1x1_014045_TTUQ1b1x1_3802_OrAsAjzk/fd_Cam-09-Q1b1x1_2026-01-17_23-54-32_20.00sec_-15.00C_LIGHT_0241.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-09-Q1b1x1_014045_TTUQ1b1x1_3802_OrAsAjzk/fd_Cam-09-Q1b1x1_2026-01-17_23-55-30_20.00sec_-15.00C_LIGHT_0242.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:32.60 +63:26:27.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-17_23-55-30_20_00sec_-15_00C_LIGHT_0242_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-17_23-54-32_20_00sec_-15_00C_LIGHT_0241_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-17_23-55-30_20_00sec_-15_00C_LIGHT_0242_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-17_23-54-32_20_00sec_-15_00C_LIGHT_0241_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2467 2461058.7467 14.42 04:08:36.26 +60:13:29.7
145.18107 6.17305 galactic Cam Second-epoch detections are separated by 3.2" 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 | ASASSN-V J040841.69+601353.2 | 04:08:41.69 +60:13:53.2 (Gaia DR3) | SRS (local) | 2458707.09000 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J040841.69+601353.2,2461058.7467,14.42,0.05,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
ASASSN-V J040841.69+601353.2 20260118.2467 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2025-12-23_02-00-56_20.00sec_-15.00C_LIGHT_0407.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-09-Q1b1x1_014045_TTUQ1b1x1_3802_OrAsAjzk/fd_Cam-09-Q1b1x1_2026-01-17_23-54-32_20.00sec_-15.00C_LIGHT_0241.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-09-Q1b1x1_014045_TTUQ1b1x1_3802_OrAsAjzk/fd_Cam-09-Q1b1x1_2026-01-17_23-55-30_20.00sec_-15.00C_LIGHT_0242.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:08:36.26 +60:13:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-17_23-55-30_20_00sec_-15_00C_LIGHT_0242_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-17_23-54-32_20_00sec_-15_00C_LIGHT_0241_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-17_23-55-30_20_00sec_-15_00C_LIGHT_0242_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-17_23-54-32_20_00sec_-15_00C_LIGHT_0241_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2071 2461058.7071 14.49 01:59:12.60 +47:10:26.7
134.71986 -14.14057 galactic And Second-epoch detections are separated by 1.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.8182+47.1680 | 01:59:12.60 +47:10:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.2071* 01 59 12.60 +47 10 26.7 14.5 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
ATO J029.8182+47.1680,2461058.7071,14.49,0.05,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 J029.8182+47.1680 20260118.2071 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/And-03-Q1b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_And-03-Q1b1x1_021859_TTUQ1b1x1_7148_xuubb4ZQ/fd_And-03-Q1b1x1_2026-01-17_22-57-37_20.00sec_-14.90C_LIGHT_0184.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_And-03-Q1b1x1_021859_TTUQ1b1x1_7148_xuubb4ZQ/fd_And-03-Q1b1x1_2026-01-17_22-58-34_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:12.60 +47:10:26.7 ;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_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-01-17_22-58-34_20_00sec_-15_00C_LIGHT_0185_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_2026-01-17_22-57-37_20_00sec_-14_90C_LIGHT_0184_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_2026-01-17_22-58-34_20_00sec_-15_00C_LIGHT_0185_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_2026-01-17_22-57-37_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2071 2461058.7071 14.44 02:12:06.32 +50:32:09.3
135.80076 -10.30928 galactic And Second-epoch detections are separated by 4.0" 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 358705772957372032 | 02:12:09.52 +50:32:09.3 (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 01 18.2071* 02 12 06.32 +50 32 09.3 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
Gaia DR3 358705772957372032,2461058.7071,14.44,0.05,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
Gaia DR3 358705772957372032 20260118.2071 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 /mnt/usb2/NMW-TexasTech/reference_imgs/And-03-Q1b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_And-03-Q1b1x1_021859_TTUQ1b1x1_7148_xuubb4ZQ/fd_And-03-Q1b1x1_2026-01-17_22-57-37_20.00sec_-14.90C_LIGHT_0184.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_And-03-Q1b1x1_021859_TTUQ1b1x1_7148_xuubb4ZQ/fd_And-03-Q1b1x1_2026-01-17_22-58-34_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:12:06.32 +50:32:09.3 ;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_2026-01-17_22-58-34_20_00sec_-15_00C_LIGHT_0185_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_2026-01-17_22-57-37_20_00sec_-14_90C_LIGHT_0184_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_2026-01-17_22-58-34_20_00sec_-15_00C_LIGHT_0185_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_2026-01-17_22-57-37_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2071 2461058.7071 14.44 02:25:00.85 +48:44:23.8
138.41903 -11.29762 galactic And Second-epoch detections are separated by 0.8" and 8.7 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 J036.2705+48.7327 | 02:25:05.28 +48:44:38.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.2071* 02 25 00.85 +48 44 23.8 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 J036.2705+48.7327,2461058.7071,14.44,0.05,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 J036.2705+48.7327 20260118.2071 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 /mnt/usb2/NMW-TexasTech/reference_imgs/And-03-Q1b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_And-03-Q1b1x1_021859_TTUQ1b1x1_7148_xuubb4ZQ/fd_And-03-Q1b1x1_2026-01-17_22-57-37_20.00sec_-14.90C_LIGHT_0184.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_And-03-Q1b1x1_021859_TTUQ1b1x1_7148_xuubb4ZQ/fd_And-03-Q1b1x1_2026-01-17_22-58-34_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:25:00.85 +48:44:23.8 ;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_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-01-17_22-58-34_20_00sec_-15_00C_LIGHT_0185_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_2026-01-17_22-57-37_20_00sec_-14_90C_LIGHT_0184_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_2026-01-17_22-58-34_20_00sec_-15_00C_LIGHT_0185_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_2026-01-17_22-57-37_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1228 2461058.6228 11.83 21:11:32.36 +35:54:41.1
80.82967 -8.41017 galactic Cyg Second-epoch detections are separated by 1.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.8896+35.9161 | 21:11:32.42 +35:54:32.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J317.8896+35.9161,2461058.6228,11.83,0.05,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
ATO J317.8896+35.9161 20260118.1228 11.83CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20.00sec_-15.00C_LIGHT_0064.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:11:32.36 +35:54:41.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1228 2461058.6228 11.35 21:13:20.64 +35:59:08.9
81.13541 -8.62814 galactic Cyg Second-epoch detections are separated by 0.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1867711338071923072 | 21:13:20.59 +35:59:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.899+/-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 1867711338071923072,2461058.6228,11.35,0.05,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 1867711338071923072 20260118.1228 11.35CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20.00sec_-15.00C_LIGHT_0064.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:13:20.64 +35:59:08.9 ;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_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1228 2461058.6228 10.21 21:14:09.86 +34:19:14.8
80.01363 -9.88299 galactic Cyg Second-epoch detections are separated by 0.5" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.5384+34.3116 | 21:14:09.91 +34:19:15.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.537+/-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
ATO J318.5384+34.3116,2461058.6228,10.21,0.05,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 J318.5384+34.3116 20260118.1228 10.21CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20.00sec_-15.00C_LIGHT_0064.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:14:09.86 +34:19:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1228 2461058.6228 9.69 21:17:16.01 +34:27:59.7
80.56565 -10.25106 galactic Cyg Second-epoch detections are separated by 0.9" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1867309260410028800 | 21:17:15.96 +34:27:59.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.719+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1867309260410028800,2461058.6228,9.69,0.05,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
Gaia DR3 1867309260410028800 20260118.1228 9.69CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20.00sec_-15.00C_LIGHT_0064.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:17:16.01 +34:27:59.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1228 2461058.6228 10.91 21:15:42.53 +33:39:27.4
79.74118 -10.56884 galactic Cyg Second-epoch detections are separated by 0.5" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J318.9388+33.6591 | 21:15:42.55 +33:39:28.4 (Gaia DR3) | SINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.144+/-0.031 (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
ATO J318.9388+33.6591,2461058.6228,10.91,0.05,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 J318.9388+33.6591 20260118.1228 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20.00sec_-15.00C_LIGHT_0064.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:15:42.53 +33:39:27.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1228 2461058.6228 10.86 21:10:29.59 +37:37:41.2
81.96312 -7.09501 galactic Cyg Second-epoch detections are separated by 0.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J317.6191+37.6397 | 21:10:29.72 +37:37:39.0 (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 J317.6191+37.6397,2461058.6228,10.86,0.05,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
ATO J317.6191+37.6397 20260118.1228 10.86CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20.00sec_-15.00C_LIGHT_0064.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:10:29.59 +37:37:41.2 ;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_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1228 2461058.6228 10.71 21:18:15.64 +34:18:30.0
80.59199 -10.50876 galactic Cyg Second-epoch detections are separated by 0.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1855298848224306048 | 21:18:15.61 +34:18:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.904+/-0.034 (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 1855298848224306048,2461058.6228,10.71,0.05,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
Gaia DR3 1855298848224306048 20260118.1228 10.71CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-19-48_20.00sec_-15.00C_LIGHT_0040.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-07-Q1b1x1_2025-12-22_20-20-53_20.00sec_-14.90C_LIGHT_0041.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20.00sec_-15.00C_LIGHT_0064.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-17_CI_Cyg-07-Q1b1x1_222330_TTUQ1b1x1_26646_sZmuGn6C/fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20.00sec_-14.90C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:18:15.64 +34:18:30.0 ;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_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-59_20_00sec_-14_90C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-07-Q1b1x1_2025-12-22_20-19-48_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png resample_wcs_fd_Cyg-07-Q1b1x1_2026-01-17_20-56-19_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3228 2461058.8228 12.35 10:22:06.47 +48:30:53.2
166.21561 54.13109 galactic UMa Second-epoch detections are separated by 0.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 834690992346732416 | 10:22:06.55 +48:30:53.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.238+/-0.027 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3228* 10 22 06.47 +48 30 53.2 12.3 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
Gaia DR3 834690992346732416,2461058.8228,12.35,0.05,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
Gaia DR3 834690992346732416 20260118.3228 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 /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-09-Q1b1x1_2025-12-23_05-03-39_20.00sec_-15.00C_LIGHT_0598.fits /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-09-Q1b1x1_2025-12-23_05-04-50_20.00sec_-14.90C_LIGHT_0599.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_UMa-09-Q1b1x1_022635_TTUQ1b1x1_16896_9FLl2EYK/fd_UMa-09-Q1b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_UMa-09-Q1b1x1_022635_TTUQ1b1x1_16896_9FLl2EYK/fd_UMa-09-Q1b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:22:06.47 +48:30:53.2 ;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_UMa-09-Q1b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q1b1x1_2026-01-18_01-45-00_20_00sec_-15_00C_LIGHT_0333_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-09-Q1b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q1b1x1_2026-01-18_01-44-14_20_00sec_-15_00C_LIGHT_0332_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q1b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q1b1x1_2026-01-18_01-45-00_20_00sec_-15_00C_LIGHT_0333_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q1b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q1b1x1_2026-01-18_01-44-14_20_00sec_-15_00C_LIGHT_0332_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3311 2461058.8311 11.25 16:19:11.76 +40:53:49.9
64.81388 45.50136 galactic Her Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1380829653498924160 | 16:19:12.19 +40:53:46.0 (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 01 18.3311* 16 19 11.76 +40 53 49.9 11.2 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 1380829653498924160,2461058.8311,11.25,0.05,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
Gaia DR3 1380829653498924160 20260118.3311 11.25CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-28-54_20.00sec_-15.00C_LIGHT_0626.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20.00sec_-15.00C_LIGHT_0344.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20.00sec_-14.90C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:19:11.76 +40:53:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3311 2461058.8311 11.68 16:18:47.03 +40:50:59.1
64.74848 45.58025 galactic Her Second-epoch detections are separated by 1.3" 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 1380808522259324416 | 16:18:47.80 +40:50:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3311* 16 18 47.03 +40 50 59.1 11.7 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 1380808522259324416,2461058.8311,11.68,0.05,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
Gaia DR3 1380808522259324416 20260118.3311 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-28-54_20.00sec_-15.00C_LIGHT_0626.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20.00sec_-15.00C_LIGHT_0344.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20.00sec_-14.90C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:18:47.03 +40:50:59.1 ;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_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3311 2461058.8311 11.09 16:18:23.57 +41:59:20.5
66.37931 45.61724 galactic Her Second-epoch detections are separated by 0.9" 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 1381672596669084928 | 16:18:23.63 +41:59:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.928+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3311* 16 18 23.57 +41 59 20.5 11.1 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 1381672596669084928,2461058.8311,11.09,0.05,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
Gaia DR3 1381672596669084928 20260118.3311 11.09CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-28-54_20.00sec_-15.00C_LIGHT_0626.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-29-35_20.00sec_-14.90C_LIGHT_0627.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20.00sec_-15.00C_LIGHT_0344.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20.00sec_-14.90C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:18:23.57 +41:59:20.5 ;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_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3311 2461058.8311 10.62 15:59:27.10 +40:53:51.9
65.09414 49.22714 galactic Her Second-epoch detections are separated by 0.5" 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 J239.8574+40.9056 | 15:59:27.12 +40:53:51.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.815+/-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!
TCP 2026 01 18.3311* 15 59 27.10 +40 53 51.9 10.6 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
ATO J239.8574+40.9056,2461058.8311,10.62,0.05,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
ATO J239.8574+40.9056 20260118.3311 10.62CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-28-54_20.00sec_-15.00C_LIGHT_0626.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-29-35_20.00sec_-14.90C_LIGHT_0627.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20.00sec_-15.00C_LIGHT_0344.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20.00sec_-14.90C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:59:27.10 +40:53:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3311 2461058.8311 12.72 16:20:15.19 +43:44:53.6
68.85414 45.17974 galactic Her Second-epoch detections are separated by 0.5" 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 1382393777508355456 | 16:20:15.26 +43:44:55.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3311* 16 20 15.19 +43 44 53.6 12.7 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 1382393777508355456,2461058.8311,12.72,0.05,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
Gaia DR3 1382393777508355456 20260118.3311 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-28-54_20.00sec_-15.00C_LIGHT_0626.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-29-35_20.00sec_-14.90C_LIGHT_0627.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20.00sec_-15.00C_LIGHT_0344.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20.00sec_-14.90C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:20:15.19 +43:44:53.6 ;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_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3311 2461058.8311 13.35 16:11:07.13 +43:46:02.1
69.07829 46.82180 galactic Her Second-epoch detections are separated by 0.9" 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 J242.7699+43.7727 | 16:11:07.13 +43:46:02.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.370+/-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!
TCP 2026 01 18.3311* 16 11 07.13 +43 46 02.1 13.3 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
ATO J242.7699+43.7727,2461058.8311,13.35,0.05,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
ATO J242.7699+43.7727 20260118.3311 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-28-54_20.00sec_-15.00C_LIGHT_0626.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-29-35_20.00sec_-14.90C_LIGHT_0627.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20.00sec_-15.00C_LIGHT_0344.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20.00sec_-14.90C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:11:07.13 +43:46:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3311 2461058.8311 12.06 16:19:06.25 +42:36:26.0
67.25209 45.45682 galactic Her Second-epoch detections are separated by 1.1" 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 | ASASSN-V J161907.07+423553.5 | 16:19:07.00 +42:35:53.4 (Gaia DR3) | SR (local) | 54.700000000000 (local) | Gaia3var=VARIABLE J-Ks=0.275+/-0.025 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3311* 16 19 06.25 +42 36 26.0 12.1 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
ASASSN-V J161907.07+423553.5,2461058.8311,12.06,0.05,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
ASASSN-V J161907.07+423553.5 20260118.3311 12.06CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-28-54_20.00sec_-15.00C_LIGHT_0626.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-03-Q1b1x1_2025-12-23_05-29-35_20.00sec_-14.90C_LIGHT_0627.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20.00sec_-15.00C_LIGHT_0344.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-03-Q1b1x1_023640_TTUQ1b1x1_12570_lbqCU73r/fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20.00sec_-14.90C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:19:06.25 +42:36:26.0 ;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_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-58_20_00sec_-14_90C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-03-Q1b1x1_2025-12-23_05-28-54_20_00sec_-15_00C_LIGHT_0626_fits__*pix.png resample_wcs_fd_Boo-03-Q1b1x1_2026-01-18_01-56-16_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2348 2461058.7348 14.43 06:03:35.60 +35:56:16.7
175.84043 6.79295 galactic Aur Second-epoch detections are separated by 7.5" and 1.2 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 3453531667404204800 | 06:03:36.81 +35:56:46.6 (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 3453531667404204800,2461058.7348,14.43,0.05,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
Gaia DR3 3453531667404204800 20260118.2348 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Aur-04-Q1b1x1_024644_TTUQ1b1x1_14226_MLSu0M0z/fd_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Aur-04-Q1b1x1_024644_TTUQ1b1x1_14226_MLSu0M0z/fd_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:35.60 +35:56:16.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-17_23-38-14_20_00sec_-14_90C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-17_23-37-37_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-17_23-38-14_20_00sec_-14_90C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-17_23-37-37_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2348 2461058.7348 14.41 06:16:49.93 +40:23:52.5
173.05383 11.16095 galactic Aur Second-epoch detections are separated by 2.7" 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 | Gaia DR3 959831805185509120 | 06:16:51.31 +40:24:15.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 959831805185509120,2461058.7348,14.41,0.05,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
Gaia DR3 959831805185509120 20260118.2348 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Aur-04-Q1b1x1_024644_TTUQ1b1x1_14226_MLSu0M0z/fd_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Aur-04-Q1b1x1_024644_TTUQ1b1x1_14226_MLSu0M0z/fd_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:49.93 +40:23:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-17_23-38-14_20_00sec_-14_90C_LIGHT_0225_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-17_23-37-37_20_00sec_-14_90C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-17_23-38-14_20_00sec_-14_90C_LIGHT_0225_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-17_23-37-37_20_00sec_-14_90C_LIGHT_0224_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3198 2461058.8198 10.09 16:17:18.36 +50:00:36.3
77.73768 44.88308 galactic Her 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 1423532039421321728 | 16:17:18.38 +50:00:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1927AnHar.100...33C HD 234295 J-Ks=0.223+/-0.029 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3198* 16 17 18.36 +50 00 36.3 10.1 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 1423532039421321728,2461058.8198,10.09,0.05,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
Gaia DR3 1423532039421321728 20260118.3198 10.09CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-09-Q1b1x1_2025-12-23_05-11-49_20.00sec_-15.00C_LIGHT_0606.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-09-Q1b1x1_021059_TTUQ1b1x1_23550_PqXMQo7Y/fd_Dra-09-Q1b1x1_2026-01-18_01-39-52_20.00sec_-14.90C_LIGHT_0328.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-09-Q1b1x1_021059_TTUQ1b1x1_23550_PqXMQo7Y/fd_Dra-09-Q1b1x1_2026-01-18_01-40-53_20.00sec_-14.90C_LIGHT_0329.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:17:18.36 +50:00:36.3 ;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_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-01-18_01-40-53_20_00sec_-14_90C_LIGHT_0329_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_2026-01-18_01-39-52_20_00sec_-14_90C_LIGHT_0328_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_2026-01-18_01-40-53_20_00sec_-14_90C_LIGHT_0329_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_2026-01-18_01-39-52_20_00sec_-14_90C_LIGHT_0328_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3198 2461058.8198 12.70 16:08:46.88 +49:33:29.2
77.49477 46.32137 galactic Her Second-epoch detections are separated by 0.7" 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 | target | 16:08:46.88 +49:33:29.2 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.026 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3198* 16 08 46.88 +49 33 29.2 12.7 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
target,2461058.8198,12.70,0.05,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
target 20260118.3198 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-09-Q1b1x1_2025-12-23_05-11-49_20.00sec_-15.00C_LIGHT_0606.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-09-Q1b1x1_2025-12-23_05-12-29_20.00sec_-15.00C_LIGHT_0607.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-09-Q1b1x1_021059_TTUQ1b1x1_23550_PqXMQo7Y/fd_Dra-09-Q1b1x1_2026-01-18_01-39-52_20.00sec_-14.90C_LIGHT_0328.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-09-Q1b1x1_021059_TTUQ1b1x1_23550_PqXMQo7Y/fd_Dra-09-Q1b1x1_2026-01-18_01-40-53_20.00sec_-14.90C_LIGHT_0329.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:08:46.88 +49:33:29.2 ;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_2026-01-18_01-40-53_20_00sec_-14_90C_LIGHT_0329_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_2026-01-18_01-39-52_20_00sec_-14_90C_LIGHT_0328_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_2026-01-18_01-40-53_20_00sec_-14_90C_LIGHT_0329_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_2026-01-18_01-39-52_20_00sec_-14_90C_LIGHT_0328_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2318 2461058.7318 14.38 05:24:46.27 +40:55:24.3
167.60783 2.88977 galactic Aur Second-epoch detections are separated by 2.8" 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 | ATO J081.1932+40.9218 | 05:24:42.82 +40:55:36.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.1932+40.9218,2461058.7318,14.38,0.05,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
ATO J081.1932+40.9218 20260118.2318 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2025-12-23_02-30-08_20.00sec_-15.00C_LIGHT_0433.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Aur-02-Q1b1x1_022101_TTUQ1b1x1_16923_If0r91Xz/fd_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Aur-02-Q1b1x1_022101_TTUQ1b1x1_16923_If0r91Xz/fd_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:46.27 +40:55:24.3 ;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_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-17_23-34-12_20_00sec_-15_00C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-17_23-33-08_20_00sec_-15_00C_LIGHT_0220_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-17_23-34-12_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-17_23-33-08_20_00sec_-15_00C_LIGHT_0220_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2318 2461058.7318 14.38 05:13:48.76 +50:59:48.3
158.20692 7.05965 galactic Aur Second-epoch detections are separated by 0.6" 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 J078.4613+50.9888 | 05:13:48.76 +50:59:48.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J078.4613+50.9888,2461058.7318,14.38,0.05,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
ATO J078.4613+50.9888 20260118.2318 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2025-12-23_02-30-08_20.00sec_-15.00C_LIGHT_0433.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Aur-02-Q1b1x1_022101_TTUQ1b1x1_16923_If0r91Xz/fd_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Aur-02-Q1b1x1_022101_TTUQ1b1x1_16923_If0r91Xz/fd_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:48.76 +50:59:48.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-17_23-34-12_20_00sec_-15_00C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-17_23-33-08_20_00sec_-15_00C_LIGHT_0220_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-17_23-34-12_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-17_23-33-08_20_00sec_-15_00C_LIGHT_0220_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2522 2461058.7522 13.12 08:34:19.70 +34:19:25.2
188.47525 35.17807 galactic Lyn Second-epoch detections are separated by 0.2" and 8.8 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 J128.5930+34.3180 | 08:34:19.70 +34:19:25.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.352+/-0.028 (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 J128.5930+34.3180,2461058.7522,13.12,0.05,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 J128.5930+34.3180 20260118.2522 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-02-Q1b1x1_2025-12-23_03-37-29_20.00sec_-14.90C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-02-Q1b1x1_031432_TTUQ1b1x1_23585_jjapmCwi/fd_Gem-02-Q1b1x1_2026-01-18_00-02-34_20.00sec_-14.90C_LIGHT_0249.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-02-Q1b1x1_031432_TTUQ1b1x1_23585_jjapmCwi/fd_Gem-02-Q1b1x1_2026-01-18_00-03-19_20.00sec_-14.90C_LIGHT_0250.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:34:19.70 +34:19:25.2 ;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_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-01-18_00-03-19_20_00sec_-14_90C_LIGHT_0250_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-01-18_00-02-34_20_00sec_-14_90C_LIGHT_0249_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-01-18_00-03-19_20_00sec_-14_90C_LIGHT_0250_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q1b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q1b1x1_2026-01-18_00-02-34_20_00sec_-14_90C_LIGHT_0249_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3529 2461058.8529 13.05 15:33:58.53 +26:11:58.3
40.96278 53.83511 galactic CrB Second-epoch detections are separated by 0.5" 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 1222593948686491648 | 15:33:59.79 +26:12:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.820+/-0.031 (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 1222593948686491648,2461058.8529,13.05,0.05,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 1222593948686491648 20260118.3529 13.05CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-06-Q1b1x1_2025-12-23_06-23-30_20.00sec_-15.00C_LIGHT_0686.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-06-Q1b1x1_2025-12-23_06-24-12_20.00sec_-15.00C_LIGHT_0687.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-06-Q1b1x1_032831_TTUQ1b1x1_30960_mZ16Zbb5/fd_Boo-06-Q1b1x1_2026-01-18_02-27-38_20.00sec_-15.00C_LIGHT_0376.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-06-Q1b1x1_032831_TTUQ1b1x1_30960_mZ16Zbb5/fd_Boo-06-Q1b1x1_2026-01-18_02-28-30_20.00sec_-15.00C_LIGHT_0377.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:33:58.53 +26:11:58.3 ;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_Boo-06-Q1b1x1_2025-12-23_06-23-30_20_00sec_-15_00C_LIGHT_0686_fits__*pix.png resample_wcs_fd_Boo-06-Q1b1x1_2026-01-18_02-28-30_20_00sec_-15_00C_LIGHT_0377_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-06-Q1b1x1_2025-12-23_06-23-30_20_00sec_-15_00C_LIGHT_0686_fits__*pix.png resample_wcs_fd_Boo-06-Q1b1x1_2026-01-18_02-27-38_20_00sec_-15_00C_LIGHT_0376_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-06-Q1b1x1_2025-12-23_06-23-30_20_00sec_-15_00C_LIGHT_0686_fits__*pix.png resample_wcs_fd_Boo-06-Q1b1x1_2026-01-18_02-28-30_20_00sec_-15_00C_LIGHT_0377_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-06-Q1b1x1_2025-12-23_06-23-30_20_00sec_-15_00C_LIGHT_0686_fits__*pix.png resample_wcs_fd_Boo-06-Q1b1x1_2026-01-18_02-27-38_20_00sec_-15_00C_LIGHT_0376_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3559 2461058.8559 14.43 10:42:38.12 +23:57:05.7
211.91061 60.85144 galactic LMi Second-epoch detections are separated by 0.2" 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 | target | 10:42:38.12 +23:57:05.7 (user input) | T | P | (position from user input) J-Ks=1.081+/-0.100 (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
target,2461058.8559,14.43,0.05,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
target 20260118.3559 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Leo-02-Q1b1x1_034241_TTUQ1b1x1_12586_GHlhFS3D/fd_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Leo-02-Q1b1x1_034241_TTUQ1b1x1_12586_GHlhFS3D/fd_Leo-02-Q1b1x1_2026-01-18_02-32-46_20.00sec_-14.90C_LIGHT_0381.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:42:38.12 +23:57:05.7 ;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_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-01-18_02-32-46_20_00sec_-14_90C_LIGHT_0381_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_2026-01-18_02-32-00_20_00sec_-15_00C_LIGHT_0380_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_2026-01-18_02-32-46_20_00sec_-14_90C_LIGHT_0381_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_2026-01-18_02-32-00_20_00sec_-15_00C_LIGHT_0380_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1835 2461058.6835 12.29 03:55:37.77 -20:39:19.3
214.44591 -47.63289 galactic Eri Second-epoch detections are separated by 0.6" 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 5093904163077230336 | 03:55:37.79 -20:39:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-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!
TCP 2026 01 18.1835* 03 55 37.77 -20 39 19.3 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
Gaia DR3 5093904163077230336,2461058.6835,12.29,0.05,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 5093904163077230336 20260118.1835 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Eri-07-Q1b1x1_2025-12-22_22-47-30_20.00sec_-15.00C_LIGHT_0196.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Eri-07-Q1b1x1_2025-12-22_22-48-23_20.00sec_-15.00C_LIGHT_0197.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Eri-07-Q1b1x1_001745_TTUQ1b1x1_29442_qxsc3yEb/fd_Eri-07-Q1b1x1_2026-01-17_22-23-43_20.00sec_-15.00C_LIGHT_0150.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Eri-07-Q1b1x1_001745_TTUQ1b1x1_29442_qxsc3yEb/fd_Eri-07-Q1b1x1_2026-01-17_22-24-29_20.00sec_-15.00C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:37.77 -20:39:19.3 ;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_Eri-07-Q1b1x1_2025-12-22_22-47-30_20_00sec_-15_00C_LIGHT_0196_fits__*pix.png resample_wcs_fd_Eri-07-Q1b1x1_2026-01-17_22-24-29_20_00sec_-15_00C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-07-Q1b1x1_2025-12-22_22-47-30_20_00sec_-15_00C_LIGHT_0196_fits__*pix.png resample_wcs_fd_Eri-07-Q1b1x1_2026-01-17_22-23-43_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_Eri-07-Q1b1x1_2025-12-22_22-47-30_20_00sec_-15_00C_LIGHT_0196_fits__*pix.png resample_wcs_fd_Eri-07-Q1b1x1_2026-01-17_22-24-29_20_00sec_-15_00C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-07-Q1b1x1_2025-12-22_22-47-30_20_00sec_-15_00C_LIGHT_0196_fits__*pix.png resample_wcs_fd_Eri-07-Q1b1x1_2026-01-17_22-23-43_20_00sec_-15_00C_LIGHT_0150_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.1835 2461058.6835 12.90 03:56:42.29 -22:06:28.5
216.61849 -47.82569 galactic Eri Second-epoch detections are separated by 1.5" 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 | target | 03:56:42.29 -22:06:28.5 (user input) | T | P | (position from user input) J-Ks=0.551+/-0.035 (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 01 18.1835* 03 56 42.29 -22 06 28.5 12.9 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
target,2461058.6835,12.90,0.05,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 20260118.1835 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Eri-07-Q1b1x1_2025-12-22_22-47-30_20.00sec_-15.00C_LIGHT_0196.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Eri-07-Q1b1x1_2025-12-22_22-48-23_20.00sec_-15.00C_LIGHT_0197.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Eri-07-Q1b1x1_001745_TTUQ1b1x1_29442_qxsc3yEb/fd_Eri-07-Q1b1x1_2026-01-17_22-23-43_20.00sec_-15.00C_LIGHT_0150.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Eri-07-Q1b1x1_001745_TTUQ1b1x1_29442_qxsc3yEb/fd_Eri-07-Q1b1x1_2026-01-17_22-24-29_20.00sec_-15.00C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:42.29 -22:06:28.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-07-Q1b1x1_2025-12-22_22-47-30_20_00sec_-15_00C_LIGHT_0196_fits__*pix.png resample_wcs_fd_Eri-07-Q1b1x1_2026-01-17_22-24-29_20_00sec_-15_00C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-07-Q1b1x1_2025-12-22_22-47-30_20_00sec_-15_00C_LIGHT_0196_fits__*pix.png resample_wcs_fd_Eri-07-Q1b1x1_2026-01-17_22-23-43_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_Eri-07-Q1b1x1_2025-12-22_22-47-30_20_00sec_-15_00C_LIGHT_0196_fits__*pix.png resample_wcs_fd_Eri-07-Q1b1x1_2026-01-17_22-24-29_20_00sec_-15_00C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-07-Q1b1x1_2025-12-22_22-47-30_20_00sec_-15_00C_LIGHT_0196_fits__*pix.png resample_wcs_fd_Eri-07-Q1b1x1_2026-01-17_22-23-43_20_00sec_-15_00C_LIGHT_0150_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2088 2461058.7088 13.57 06:16:26.75 -21:22:32.2
228.69518 -16.99233 galactic CMa Second-epoch detections are separated by 1.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J094.1097-21.3731 | 06:16:26.75 -21:22:32.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.1097-21.3731,2461058.7088,13.57,0.05,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
ATO J094.1097-21.3731 20260118.2088 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-01-Q1b1x1_2025-12-22_23-57-47_20.00sec_-15.00C_LIGHT_0276.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMa-01-Q1b1x1_002144_TTUQ1b1x1_11550_Ek69Ds0O/fd_CMa-01-Q1b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMa-01-Q1b1x1_002144_TTUQ1b1x1_11550_Ek69Ds0O/fd_CMa-01-Q1b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:26.75 -21:22:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-01-Q1b1x1_2025-12-22_23-57-47_20_00sec_-15_00C_LIGHT_0276_fits__*pix.png resample_wcs_fd_CMa-01-Q1b1x1_2026-01-17_23-01-02_20_00sec_-14_90C_LIGHT_0187_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_2026-01-17_22-59-59_20_00sec_-15_00C_LIGHT_0186_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_2026-01-17_23-01-02_20_00sec_-14_90C_LIGHT_0187_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_2026-01-17_22-59-59_20_00sec_-15_00C_LIGHT_0186_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3624 2461058.8624 11.68 16:34:27.59 +25:38:47.1
44.59962 40.45397 galactic Her Second-epoch detections are separated by 2.8" and 8.8 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 1300966076660091776 | 16:34:28.27 +25:38:41.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3624* 16 34 27.59 +25 38 47.1 11.7 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 1300966076660091776,2461058.8624,11.68,0.05,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
Gaia DR3 1300966076660091776 20260118.3624 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-02-Q1b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-02-Q1b1x1_033032_TTUQ1b1x1_15628_aRUl6Of3/fd_CrB-02-Q1b1x1_2026-01-18_02-41-22_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-02-Q1b1x1_033032_TTUQ1b1x1_15628_aRUl6Of3/fd_CrB-02-Q1b1x1_2026-01-18_02-42-03_20.00sec_-15.00C_LIGHT_0391.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:34:27.59 +25:38:47.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q1b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_fd_CrB-02-Q1b1x1_2026-01-18_02-42-03_20_00sec_-15_00C_LIGHT_0391_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q1b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_fd_CrB-02-Q1b1x1_2026-01-18_02-41-22_20_00sec_-15_00C_LIGHT_0390_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q1b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_fd_CrB-02-Q1b1x1_2026-01-18_02-42-03_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q1b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_fd_CrB-02-Q1b1x1_2026-01-18_02-41-22_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3624 2461058.8624 11.86 16:33:57.32 +25:04:42.3
43.84006 40.41691 galactic Her Second-epoch detections are separated by 0.9" 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 1300911547755051520 | 16:33:57.77 +25:04:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3624* 16 33 57.32 +25 04 42.3 11.9 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 1300911547755051520,2461058.8624,11.86,0.05,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
Gaia DR3 1300911547755051520 20260118.3624 11.86CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-02-Q1b1x1_2025-12-23_06-30-32_20.00sec_-15.00C_LIGHT_0694.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-02-Q1b1x1_033032_TTUQ1b1x1_15628_aRUl6Of3/fd_CrB-02-Q1b1x1_2026-01-18_02-41-22_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-02-Q1b1x1_033032_TTUQ1b1x1_15628_aRUl6Of3/fd_CrB-02-Q1b1x1_2026-01-18_02-42-03_20.00sec_-15.00C_LIGHT_0391.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:33:57.32 +25:04:42.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-02-Q1b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_fd_CrB-02-Q1b1x1_2026-01-18_02-42-03_20_00sec_-15_00C_LIGHT_0391_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-02-Q1b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_fd_CrB-02-Q1b1x1_2026-01-18_02-41-22_20_00sec_-15_00C_LIGHT_0390_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q1b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_fd_CrB-02-Q1b1x1_2026-01-18_02-42-03_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-02-Q1b1x1_2025-12-23_06-30-32_20_00sec_-15_00C_LIGHT_0694_fits__*pix.png resample_wcs_fd_CrB-02-Q1b1x1_2026-01-18_02-41-22_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3663 2461058.8663 14.18 14:19:12.71 +24:47:54.7
31.13178 70.15965 galactic Boo Second-epoch detections are separated by 4.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J214.8033+24.7987 | 14:19:12.71 +24:47:54.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.157+/-0.051 (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
ATO J214.8033+24.7987,2461058.8663,14.18,0.05,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
ATO J214.8033+24.7987 20260118.3663 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-01-09_03-39-22_20.00sec_-15.00C_LIGHT_0068.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-08-Q1b1x1_035407_TTUQ1b1x1_21490_uNyJvp7i/fd_Boo-08-Q1b1x1_2026-01-18_02-46-44_20.00sec_-14.90C_LIGHT_0396.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-08-Q1b1x1_035407_TTUQ1b1x1_21490_uNyJvp7i/fd_Boo-08-Q1b1x1_2026-01-18_02-47-51_20.00sec_-14.90C_LIGHT_0397.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:19:12.71 +24:47:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-08-Q1b1x1_2026-01-09_03-39-22_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Boo-08-Q1b1x1_2026-01-18_02-47-51_20_00sec_-14_90C_LIGHT_0397_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-08-Q1b1x1_2026-01-09_03-39-22_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Boo-08-Q1b1x1_2026-01-18_02-46-44_20_00sec_-14_90C_LIGHT_0396_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-08-Q1b1x1_2026-01-09_03-39-22_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Boo-08-Q1b1x1_2026-01-18_02-47-51_20_00sec_-14_90C_LIGHT_0397_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-08-Q1b1x1_2026-01-09_03-39-22_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Boo-08-Q1b1x1_2026-01-18_02-46-44_20_00sec_-14_90C_LIGHT_0396_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7438,14.22,0.05,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 20260118.2438 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cnc-04-Q1b1x1_040414_TTUQ1b1x1_29669_eZfeSFl2/fd_Cnc-04-Q1b1x1_2026-01-17_23-50-24_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cnc-04-Q1b1x1_040414_TTUQ1b1x1_29669_eZfeSFl2/fd_Cnc-04-Q1b1x1_2026-01-17_23-51-23_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:39.22 +16:36:33.5 ;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_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-17_23-51-23_20_00sec_-15_00C_LIGHT_0238_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-17_23-50-24_20_00sec_-15_00C_LIGHT_0237_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-17_23-51-23_20_00sec_-15_00C_LIGHT_0238_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-17_23-50-24_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 10.94 17:09:05.69 +16:53:12.5
37.57514 30.01547 galactic Her Second-epoch detections are separated by 7.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4547649743968826368 | 17:09:06.31 +16:53:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 09 05.69 +16 53 12.5 10.9 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 4547649743968826368,2461058.9107,10.94,0.05,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 4547649743968826368 20260118.4107 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:09:05.69 +16:53:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 11.29 17:10:03.69 +17:17:45.8
38.11303 29.95398 galactic Her Second-epoch detections are separated by 1.5" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4547947436743981184 | 17:10:04.08 +17:17:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 10 03.69 +17 17 45.8 11.3 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 4547947436743981184,2461058.9107,11.29,0.05,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 4547947436743981184 20260118.4107 11.29CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:10:03.69 +17:17:45.8 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 11.44 17:08:52.89 +16:49:39.5
37.48968 30.04058 galactic Her Second-epoch detections are separated by 7.8" and 9.1 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 4547647613665044992 | 17:08:53.45 +16:49:33.0 (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!
TCP 2026 01 18.4107* 17 08 52.89 +16 49 39.5 11.4 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 4547647613665044992,2461058.9107,11.44,0.05,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
Gaia DR3 4547647613665044992 20260118.4107 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:08:52.89 +16:49:39.5 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 11.57 17:10:04.52 +17:13:55.5
38.04593 29.92711 galactic Her Second-epoch detections are separated by 0.9" and 9.0 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 4547942592021167616 | 17:10:04.92 +17:13:50.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 10 04.52 +17 13 55.5 11.6 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 4547942592021167616,2461058.9107,11.57,0.05,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 4547942592021167616 20260118.4107 11.57CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:10:04.52 +17:13:55.5 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 11.71 17:10:13.28 +17:11:38.1
38.02005 29.88054 galactic Her Second-epoch detections are separated by 1.2" and 9.1 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 4547941595588446976 | 17:10:13.69 +17:11:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 10 13.28 +17 11 38.1 11.7 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 4547941595588446976,2461058.9107,11.71,0.05,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
Gaia DR3 4547941595588446976 20260118.4107 11.71CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:10:13.28 +17:11:38.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 11.79 17:09:38.95 +16:58:47.6
37.73210 29.92742 galactic Her Second-epoch detections are separated by 2.8" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4547744542486742016 | 17:09:39.30 +16:58:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 09 38.95 +16 58 47.6 11.8 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 4547744542486742016,2461058.9107,11.79,0.05,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
Gaia DR3 4547744542486742016 20260118.4107 11.79CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:09:38.95 +16:58:47.6 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 12.27 16:59:14.61 +20:09:06.5
40.17648 33.36442 galactic Her Second-epoch detections are separated by 0.6" and 9.3 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 4561499604750193536 | 16:59:14.60 +20:09:07.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 16 59 14.61 +20 09 06.5 12.3 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 4561499604750193536,2461058.9107,12.27,0.05,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
Gaia DR3 4561499604750193536 20260118.4107 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:59:14.61 +20:09:06.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 12.32 17:09:03.13 +17:05:26.0
37.78905 30.10115 galactic Her Second-epoch detections are separated by 2.7" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4547936785224930304 | 17:09:03.49 +17:05:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 09 03.13 +17 05 26.0 12.3 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 4547936785224930304,2461058.9107,12.32,0.05,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
Gaia DR3 4547936785224930304 20260118.4107 12.32CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:09:03.13 +17:05:26.0 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 12.36 17:04:22.61 +16:55:26.0
37.12495 31.07596 galactic Her Second-epoch detections are separated by 2.5" and 9.3 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 4547881191164080768 | 17:04:22.49 +16:55:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2/3: 1982ApJ...253..237C L 1277- 81
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 04 22.61 +16 55 26.0 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 4547881191164080768,2461058.9107,12.36,0.05,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
Gaia DR3 4547881191164080768 20260118.4107 12.36CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:04:22.61 +16:55:26.0 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 12.59 17:10:00.58 +16:51:41.0
37.64270 29.80306 galactic Her Second-epoch detections are separated by 3.3" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4547738903194259712 | 17:10:01.83 +16:51:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 10 00.58 +16 51 41.0 12.6 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 4547738903194259712,2461058.9107,12.59,0.05,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
Gaia DR3 4547738903194259712 20260118.4107 12.59CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:10:00.58 +16:51:41.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 12.73 17:10:05.53 +16:59:60.0
37.79934 29.83674 galactic Her Second-epoch detections are separated by 1.8" and 8.8 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 4547745229681610624 | 17:10:06.08 +16:59:52.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 10 05.53 +16 59 60.0 12.7 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 4547745229681610624,2461058.9107,12.73,0.05,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 4547745229681610624 20260118.4107 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:10:05.53 +16:59:60.0 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 12.71 17:09:39.90 +16:52:06.7
37.61464 29.88217 galactic Her Second-epoch detections are separated by 5.1" and 9.1 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 4547645994459928704 | 17:09:41.03 +16:51:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 09 39.90 +16 52 06.7 12.7 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 4547645994459928704,2461058.9107,12.71,0.05,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
Gaia DR3 4547645994459928704 20260118.4107 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:09:39.90 +16:52:06.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 12.99 17:05:19.32 +17:38:51.2
38.00766 31.13410 galactic Her Second-epoch detections are separated by 4.4" and 9.9 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 | 17:05:19.32 +17:38:51.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 05 19.32 +17 38 51.2 13.0 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
target,2461058.9107,12.99,0.05,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 20260118.4107 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:05:19.32 +17:38:51.2 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 12.96 16:55:49.70 +17:19:58.5
36.68167 33.12471 galactic Her Second-epoch detections are separated by 3.8" and 9.6 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 4558609297919492992 | 16:55:49.86 +17:19:35.8 (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 01 18.4107* 16 55 49.70 +17 19 58.5 13.0 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 4558609297919492992,2461058.9107,12.96,0.05,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
Gaia DR3 4558609297919492992 20260118.4107 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:55:49.70 +17:19:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 07 47.62 +21 59 27.6 13.0 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
target,2461058.9107,13.01,0.05,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
target 20260118.4107 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:07:47.62 +21:59:27.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 13.20 17:08:43.50 +17:02:59.0
37.71150 30.15844 galactic Her Second-epoch detections are separated by 3.9" 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 | Gaia DR3 4547842703961900288 | 17:08:43.76 +17:02:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 08 43.50 +17 02 59.0 13.2 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 4547842703961900288,2461058.9107,13.20,0.05,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
Gaia DR3 4547842703961900288 20260118.4107 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:08:43.50 +17:02:59.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 13.35 17:09:27.88 +16:49:43.1
37.55124 29.91162 galactic Her Second-epoch detections are separated by 4.5" and 8.8 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 4547648399641615488 | 17:09:28.81 +16:49:32.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4107* 17 09 27.88 +16 49 43.1 13.3 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 4547648399641615488,2461058.9107,13.35,0.05,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 4547648399641615488 20260118.4107 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:09:27.88 +16:49:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4107 2461058.9107 13.50 17:09:23.56 +16:56:46.5
37.66960 29.97170 galactic Her Second-epoch detections are separated by 8.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4547650431163591552 | 17:09:24.17 +16:56:40.3 (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 01 18.4107* 17 09 23.56 +16 56 46.5 13.5 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 4547650431163591552,2461058.9107,13.50,0.05,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
Gaia DR3 4547650431163591552 20260118.4107 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20.00sec_-15.00C_LIGHT_0461.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_035806_TTUQ1b1x1_26268_EHXKqxIP/fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20.00sec_-14.90C_LIGHT_0462.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:09:23.56 +16:56:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-51-53_20_00sec_-14_90C_LIGHT_0462_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_03-50-38_20_00sec_-15_00C_LIGHT_0461_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2301 2461058.7301 13.19 10:03:04.65 -22:25:05.5
259.39917 25.88990 galactic Hya Second-epoch detections are separated by 1.3" 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 5666723916984530560 | 10:03:05.90 -22:24:43.6 (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 5666723916984530560,2461058.7301,13.19,0.05,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 5666723916984530560 20260118.2301 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:03:04.65 -22:25:05.5 ;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-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7301,13.31,0.05,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
target 20260118.2301 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:04:53.67 -23:11:44.7 ;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-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2301 2461058.7301 13.30 10:07:20.39 -23:08:33.6
260.75217 25.98846 galactic Hya Second-epoch detections are separated by 0.8" 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 J151.8365-23.1384 | 10:07:20.39 -23:08:33.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J151.8365-23.1384,2461058.7301,13.30,0.05,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 J151.8365-23.1384 20260118.2301 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:07:20.39 -23:08:33.6 ;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_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2301 2461058.7301 13.48 10:07:30.87 -23:04:01.0
260.73138 26.07211 galactic Hya Second-epoch detections are separated by 2.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J151.8836-23.0710 | 10:07:30.87 -23:04:01.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J151.8836-23.0710,2461058.7301,13.48,0.05,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 J151.8836-23.0710 20260118.2301 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:07:30.87 -23:04:01.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7301,13.59,0.05,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
target 20260118.2301 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:05:55.18 -23:04:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7301,13.84,0.05,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
target 20260118.2301 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:07:21.69 -23:05:36.3 ;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_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2301 2461058.7301 11.77 10:14:55.87 -23:03:19.6
262.18850 27.17384 galactic Hya Second-epoch detections are separated by 0.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J153.7237-23.0507 | 10:14:55.87 -23:03:19.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.737+/-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
ATO J153.7237-23.0507,2461058.7301,11.77,0.05,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
ATO J153.7237-23.0507 20260118.2301 11.77CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-09-44_20.00sec_-15.00C_LIGHT_0471.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:14:55.87 -23:03:19.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2301 2461058.7301 11.96 10:16:28.51 -21:10:17.5
261.14983 28.85797 galactic Hya Second-epoch detections are separated by 0.6" 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 | Gaia DR3 5668071501628601216 | 10:16:28.54 -21:10:17.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.719+/-0.035 (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 5668071501628601216,2461058.7301,11.96,0.05,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
Gaia DR3 5668071501628601216 20260118.2301 11.96CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-09-44_20.00sec_-15.00C_LIGHT_0471.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:16:28.51 -21:10:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2301 2461058.7301 12.11 10:09:23.08 -21:29:50.3
259.95464 27.54533 galactic Hya Second-epoch detections are separated by 0.8" 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 5667256385553852160 | 10:09:23.11 -21:29:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.653+/-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 5667256385553852160,2461058.7301,12.11,0.05,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
Gaia DR3 5667256385553852160 20260118.2301 12.11CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-09-44_20.00sec_-15.00C_LIGHT_0471.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:23.08 -21:29:50.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2301 2461058.7301 12.46 10:12:58.48 -22:56:45.6
261.71955 26.97300 galactic Hya Second-epoch detections are separated by 0.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5666118773272604160 | 10:12:58.52 -22:56:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.036 (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 5666118773272604160,2461058.7301,12.46,0.05,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 5666118773272604160 20260118.2301 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-08-Q1b1x1_2025-12-23_03-09-44_20.00sec_-15.00C_LIGHT_0471.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20.00sec_-15.00C_LIGHT_0218.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-08-Q1b1x1_003142_TTUQ1b1x1_498_Jx6dr55W/fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20.00sec_-15.00C_LIGHT_0219.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:12:58.48 -22:56:45.6 ;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_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-31-41_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q1b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q1b1x1_2026-01-17_23-30-41_20_00sec_-15_00C_LIGHT_0218_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2634 2461058.7634 14.22 17:10:47.78 +83:51:09.0
116.53175 29.59605 galactic UMi Second-epoch detections are separated by 0.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Y UMi | 17:10:35.19 +83:50:28.4 (Gaia DR3) | M (local) | 2427892.00000 (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
Y UMi,2461058.7634,14.22,0.05,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
Y UMi 20260118.2634 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-02-Q1b1x1_2025-12-23_04-00-21_20.00sec_-15.00C_LIGHT_0526.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-02-Q1b1x1_010834_TTUQ1b1x1_7163_XeWMiSz1/fd_Cam-02-Q1b1x1_2026-01-18_00-18-37_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-02-Q1b1x1_010834_TTUQ1b1x1_7163_XeWMiSz1/fd_Cam-02-Q1b1x1_2026-01-18_00-19-32_20.00sec_-15.00C_LIGHT_0266.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:10:47.78 +83:51:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-02-Q1b1x1_2025-12-23_04-00-21_20_00sec_-15_00C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Cam-02-Q1b1x1_2026-01-18_00-19-32_20_00sec_-15_00C_LIGHT_0266_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_2026-01-18_00-18-37_20_00sec_-15_00C_LIGHT_0265_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_2026-01-18_00-19-32_20_00sec_-15_00C_LIGHT_0266_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_2026-01-18_00-18-37_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7634,14.43,0.05,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
target 20260118.2634 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-02-Q1b1x1_2025-12-23_04-00-21_20.00sec_-15.00C_LIGHT_0526.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-02-Q1b1x1_010834_TTUQ1b1x1_7163_XeWMiSz1/fd_Cam-02-Q1b1x1_2026-01-18_00-18-37_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cam-02-Q1b1x1_010834_TTUQ1b1x1_7163_XeWMiSz1/fd_Cam-02-Q1b1x1_2026-01-18_00-19-32_20.00sec_-15.00C_LIGHT_0266.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:40:53.76 +86:00:15.3 ;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_Cam-02-Q1b1x1_2025-12-23_04-00-21_20_00sec_-15_00C_LIGHT_0526_fits__*pix.png resample_wcs_fd_Cam-02-Q1b1x1_2026-01-18_00-19-32_20_00sec_-15_00C_LIGHT_0266_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_2026-01-18_00-18-37_20_00sec_-15_00C_LIGHT_0265_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_2026-01-18_00-19-32_20_00sec_-15_00C_LIGHT_0266_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_2026-01-18_00-18-37_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2508 2461058.7508 12.61 08:52:33.05 +26:10:11.4
199.42497 37.14516 galactic Cnc Second-epoch detections are separated by 0.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:52:33.05 +26:10:11.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.7508,12.61,0.05,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
target 20260118.2508 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cnc-02-Q1b1x1_033901_TTUQ1b1x1_14286_37TJub6F/fd_Cnc-02-Q1b1x1_2026-01-18_00-00-23_20.00sec_-15.00C_LIGHT_0247.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cnc-02-Q1b1x1_033901_TTUQ1b1x1_14286_37TJub6F/fd_Cnc-02-Q1b1x1_2026-01-18_00-01-32_20.00sec_-15.00C_LIGHT_0248.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:52:33.05 +26:10:11.4 ;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_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-01-18_00-01-32_20_00sec_-15_00C_LIGHT_0248_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-01-18_00-00-23_20_00sec_-15_00C_LIGHT_0247_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-01-18_00-01-32_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-01-18_00-00-23_20_00sec_-15_00C_LIGHT_0247_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2450 2461058.7450 12.78 08:36:06.46 +10:20:34.6
215.39836 27.90265 galactic Cnc Second-epoch detections are separated by 2.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 601330953705647488 | 08:36:07.02 +10:21:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 601330953705647488,2461058.7450,12.78,0.05,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
Gaia DR3 601330953705647488 20260118.2450 12.78CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20.00sec_-15.00C_LIGHT_0239.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20.00sec_-15.00C_LIGHT_0240.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:36:06.46 +10:20:34.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7450,14.37,0.05,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 20260118.2450 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20.00sec_-15.00C_LIGHT_0239.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20.00sec_-15.00C_LIGHT_0240.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:03.15 +11:05:50.4 ;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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2450 2461058.7450 14.21 08:12:39.45 +08:58:29.8
214.01142 22.09808 galactic Cnc Second-epoch detections are separated by 2.2" and 6.1 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 3098429028411075712 | 08:12:39.54 +08:59:08.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3098429028411075712,2461058.7450,14.21,0.05,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
Gaia DR3 3098429028411075712 20260118.2450 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20.00sec_-15.00C_LIGHT_0239.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20.00sec_-15.00C_LIGHT_0240.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:39.45 +08:58:29.8 ;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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2450 2461058.7450 13.13 09:04:53.83 +07:07:29.2
222.41654 32.83635 galactic Cnc Second-epoch detections are separated by 0.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:04:53.83 +07:07:29.2 (user input) | T | P | (position from user input) J-Ks=0.389+/-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
target,2461058.7450,13.13,0.05,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
target 20260118.2450 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20.00sec_-15.00C_LIGHT_0239.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20.00sec_-15.00C_LIGHT_0240.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:53.83 +07:07:29.2 ;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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2450 2461058.7450 13.04 09:01:52.65 +08:05:23.0
220.98861 32.61722 galactic Cnc Second-epoch detections are separated by 0.6" 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 | target | 09:01:52.65 +08:05:23.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.574+/-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
target,2461058.7450,13.04,0.05,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
target 20260118.2450 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20.00sec_-15.00C_LIGHT_0239.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20.00sec_-15.00C_LIGHT_0240.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:52.65 +08:05:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2450 2461058.7450 12.86 09:05:10.92 +09:35:24.0
219.82470 34.02126 galactic Cnc Second-epoch detections are separated by 0.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:05:10.92 +09:35:24.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.848+/-0.031 (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
target,2461058.7450,12.86,0.05,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
target 20260118.2450 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20.00sec_-15.00C_LIGHT_0239.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20.00sec_-15.00C_LIGHT_0240.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:10.92 +09:35:24.0 ;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-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2450 2461058.7450 13.03 08:05:02.09 +01:00:43.6
220.62649 16.79349 galactic CMi Second-epoch detections are separated by 0.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3084615520234681216 | 08:05:00.47 +01:00:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.714+/-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
Gaia DR3 3084615520234681216,2461058.7450,13.03,0.05,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 3084615520234681216 20260118.2450 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20.00sec_-15.00C_LIGHT_0239.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20.00sec_-15.00C_LIGHT_0240.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:02.09 +01:00:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2450 2461058.7450 13.00 09:05:32.75 +03:44:24.4
226.01131 31.34996 galactic Hya Second-epoch detections are separated by 0.5" 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 | target | 09:05:32.75 +03:44:24.4 (user input) | T | P | (position from user input) J-Ks=0.570+/-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
target,2461058.7450,13.00,0.05,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
target 20260118.2450 13.00CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20.00sec_-15.00C_LIGHT_0239.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-01-Q1b1x1_042612_TTUQ1b1x1_29543_iPYdFJqT/fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20.00sec_-15.00C_LIGHT_0240.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:32.75 +03:44:24.4 ;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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-53-10_20_00sec_-15_00C_LIGHT_0240_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-17_23-52-08_20_00sec_-15_00C_LIGHT_0239_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3612* 16 59 44.41 +32 44 58.2 11.2 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
target,2461058.8612,11.18,0.05,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 20260118.3612 11.18CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20.00sec_-15.00C_LIGHT_0388.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20.00sec_-15.00C_LIGHT_0389.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:59:44.41 +32:44:58.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3612 2461058.8612 11.05 15:38:08.73 +42:13:23.1
68.01739 53.00525 galactic Boo Second-epoch detections are separated by 0.6" 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 | Gaia DR3 1390322252776836736 | 15:38:09.66 +42:13:18.7 (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 1390322252776836736,2461058.8612,11.05,0.05,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 1390322252776836736 20260118.3612 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20.00sec_-15.00C_LIGHT_0388.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20.00sec_-15.00C_LIGHT_0389.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:38:08.73 +42:13:23.1 ;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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3612 2461058.8612 11.17 16:52:54.47 +32:52:25.4
54.84916 38.10324 galactic Her Second-epoch detections are separated by 4.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1313739652994809600 | 16:52:55.11 +32:52:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3612* 16 52 54.47 +32 52 25.4 11.2 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 1313739652994809600,2461058.8612,11.17,0.05,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
Gaia DR3 1313739652994809600 20260118.3612 11.17CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20.00sec_-15.00C_LIGHT_0388.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20.00sec_-15.00C_LIGHT_0389.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:52:54.47 +32:52:25.4 ;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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3612 2461058.8612 11.24 17:00:16.94 +33:47:29.5
56.34209 36.75803 galactic Her Second-epoch detections are separated by 1.1" and 3.9 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 1337869088502533504 | 17:00:17.38 +33:47:25.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3612* 17 00 16.94 +33 47 29.5 11.2 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 1337869088502533504,2461058.8612,11.24,0.05,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
Gaia DR3 1337869088502533504 20260118.3612 11.24CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20.00sec_-15.00C_LIGHT_0388.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20.00sec_-15.00C_LIGHT_0389.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:00:16.94 +33:47:29.5 ;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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3612 2461058.8612 11.62 16:57:51.76 +33:33:53.8
55.94726 37.21110 galactic Her Second-epoch detections are separated by 3.6" and 3.5 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 1313867711739655808 | 16:57:52.15 +33:33:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3612* 16 57 51.76 +33 33 53.8 11.6 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 1313867711739655808,2461058.8612,11.62,0.05,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
Gaia DR3 1313867711739655808 20260118.3612 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20.00sec_-15.00C_LIGHT_0388.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20.00sec_-15.00C_LIGHT_0389.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:57:51.76 +33:33:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3612 2461058.8612 11.96 16:58:47.26 +32:54:09.1
55.17774 36.89637 galactic Her Second-epoch detections are separated by 5.1" and 3.6 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 1313599190384258432 | 16:58:50.10 +32:53:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3612* 16 58 47.26 +32 54 09.1 12.0 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 1313599190384258432,2461058.8612,11.96,0.05,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
Gaia DR3 1313599190384258432 20260118.3612 11.96CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20.00sec_-15.00C_LIGHT_0388.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20.00sec_-15.00C_LIGHT_0389.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:58:47.26 +32:54:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3612 2461058.8612 11.92 17:00:27.86 +34:02:59.9
56.66787 36.76834 galactic Her Second-epoch detections are separated by 3.6" 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 1337882660600120832 | 17:00:28.55 +34:02:54.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3612* 17 00 27.86 +34 02 59.9 11.9 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 1337882660600120832,2461058.8612,11.92,0.05,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 1337882660600120832 20260118.3612 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20.00sec_-15.00C_LIGHT_0388.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_030432_TTUQ1b1x1_16196_JM6AdMLD/fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20.00sec_-15.00C_LIGHT_0389.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:00:27.86 +34:02:59.9 ;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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-40-21_20_00sec_-15_00C_LIGHT_0389_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_02-39-40_20_00sec_-15_00C_LIGHT_0388_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 10.46 16:14:05.15 +17:13:52.4
31.96772 42.36977 galactic Her Second-epoch detections are separated by 3.8" and 10.4 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 J243.5224+17.2183 | 16:14:05.57 +17:13:47.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0 1952CoRut..32....1H BD+17 2990
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 14 05.15 +17 13 52.4 10.5 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
ATO J243.5224+17.2183,2461058.8678,10.46,0.05,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 J243.5224+17.2183 20260118.3678 10.46CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:05.15 +17:13:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 10.72 16:14:33.13 +17:50:30.4
32.79381 42.48523 galactic Her Second-epoch detections are separated by 7.5" and 10.3 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 1199012520944491520 | 16:14:33.49 +17:50:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M4 (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 01 18.3678* 16 14 33.13 +17 50 30.4 10.7 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 1199012520944491520,2461058.8678,10.72,0.05,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 1199012520944491520 20260118.3678 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:33.13 +17:50:30.4 ;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_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 10.28 16:14:17.97 +17:11:24.2
31.94094 42.30727 galactic Her Second-epoch detections are separated by 7.2" and 10.4 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 1198765955461444864 | 16:14:18.62 +17:11:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1952CoRut..32....1H BD+17 2991
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 14 17.97 +17 11 24.2 10.3 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 1198765955461444864,2461058.8678,10.28,0.05,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
Gaia DR3 1198765955461444864 20260118.3678 10.28CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:17.97 +17:11:24.2 ;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_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 12.01 16:04:22.22 +20:02:02.9
34.52919 45.49269 galactic Her Second-epoch detections are separated by 0.5" 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 1203492446711835008 | 16:04:22.20 +20:02:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.303+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 04 22.22 +20 02 02.9 12.0 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 1203492446711835008,2461058.8678,12.01,0.05,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
Gaia DR3 1203492446711835008 20260118.3678 12.01CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:04:22.22 +20:02:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 12.52 16:13:46.41 +17:02:21.5
31.68902 42.36927 galactic Her Second-epoch detections are separated by 8.0" and 10.2 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 1198757017633739648 | 16:13:46.88 +17:02:17.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 13 46.41 +17 02 21.5 12.5 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 1198757017633739648,2461058.8678,12.52,0.05,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
Gaia DR3 1198757017633739648 20260118.3678 12.52CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:13:46.41 +17:02:21.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 13.04 16:14:28.73 +19:06:22.4
34.40033 42.93886 galactic Her Second-epoch detections are separated by 1.2" and 8.8 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 varaible 1201405126966920448 | 16:14:30.36 +19:06:16.7 (Gaia DR3) | SOLAR_LIKE (Gaia DR3) | 2022yCat.1358....0G | Gaia3var=VARIABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 14 28.73 +19 06 22.4 13.0 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 varaible 1201405126966920448,2461058.8678,13.04,0.05,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 varaible 1201405126966920448 20260118.3678 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:28.73 +19:06:22.4 ;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_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 12.95 16:15:12.35 +18:26:20.7
33.62662 42.54921 galactic Her Second-epoch detections are separated by 2.7" and 9.5 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 1200614440666497664 | 16:15:12.76 +18:26:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 15 12.35 +18 26 20.7 12.9 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 1200614440666497664,2461058.8678,12.95,0.05,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 1200614440666497664 20260118.3678 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:12.35 +18:26:20.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 13.04 16:15:01.23 +18:15:27.2
33.37487 42.52733 galactic Her Second-epoch detections are separated by 1.9" and 9.7 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 | Large-amplitude variable Gaia DR2 1200576163916014848 | 16:15:01.59 +18:15:23.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 15 01.23 +18 15 27.2 13.0 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
Large-amplitude variable Gaia DR2 1200576163916014848,2461058.8678,13.04,0.05,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
Large-amplitude variable Gaia DR2 1200576163916014848 20260118.3678 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:01.23 +18:15:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 13.07 16:14:40.11 +17:24:38.9
32.26229 42.30516 galactic Her Second-epoch detections are separated by 8.7" and 10.3 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 1198981219222620928 | 16:14:40.58 +17:24:32.7 (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 01 18.3678* 16 14 40.11 +17 24 38.9 13.1 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 1198981219222620928,2461058.8678,13.07,0.05,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
Gaia DR3 1198981219222620928 20260118.3678 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:40.11 +17:24:38.9 ;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_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 15 04.69 +18 27 18.4 13.4 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
target,2461058.8678,13.37,0.05,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 20260118.3678 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:04.69 +18:27:18.4 ;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_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3678 2461058.8678 13.27 16:15:06.37 +18:34:07.1
33.78065 42.61614 galactic Her Second-epoch detections are separated by 3.8" and 9.4 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 1200620865937592064 | 16:15:06.72 +18:34:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3678* 16 15 06.37 +18 34 07.1 13.3 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 1200620865937592064,2461058.8678,13.27,0.05,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
Gaia DR3 1200620865937592064 20260118.3678 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-01-Q1b1x1_2026-01-09_03-41-34_20.00sec_-14.90C_LIGHT_0070.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20.00sec_-15.00C_LIGHT_0398.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-01-Q1b1x1_035614_TTUQ1b1x1_25235_zmaEEMP2/fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20.00sec_-14.90C_LIGHT_0399.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:06.37 +18:34:07.1 ;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_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-50-03_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-01-Q1b1x1_2026-01-09_03-41-34_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png resample_wcs_fd_Ser-01-Q1b1x1_2026-01-18_02-48-54_20_00sec_-15_00C_LIGHT_0398_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 11.47 15:53:06.77 +34:45:00.2
55.59088 50.64146 galactic CrB Second-epoch detections are separated by 1.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1371764351926288512 | 15:53:06.69 +34:45:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2 1984AJ.....89..702L G 180- 8
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1371764351926288512,2461058.8435,11.47,0.05,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
Gaia DR3 1371764351926288512 20260118.3435 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:53:06.77 +34:45:00.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 11.79 15:53:42.01 +32:54:05.3
52.69541 50.42806 galactic CrB Second-epoch detections are separated by 1.6" and 6.1 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 1369904321849091968 | 15:53:42.43 +32:54:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1369904321849091968,2461058.8435,11.79,0.05,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
Gaia DR3 1369904321849091968 20260118.3435 11.79CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:53:42.01 +32:54:05.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 10.67 15:47:29.10 +33:34:15.1
53.64396 51.76306 galactic CrB Second-epoch detections are separated by 0.1" and 6.1 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 1370831381949887360 | 15:47:29.11 +33:34:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.031 (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 1370831381949887360,2461058.8435,10.67,0.05,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 1370831381949887360 20260118.3435 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-55-53_20.00sec_-14.90C_LIGHT_0655.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:47:29.10 +33:34:15.1 ;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_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 13.32 15:26:07.22 +41:40:23.1
67.85011 55.30561 galactic Boo Second-epoch detections are separated by 5.8" 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 J231.5332+41.6759 | 15:26:07.22 +41:40:23.1 (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 J231.5332+41.6759,2461058.8435,13.32,0.05,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 J231.5332+41.6759 20260118.3435 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:26:07.22 +41:40:23.1 ;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_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 12.21 15:53:42.19 +32:55:42.7
52.73784 50.42931 galactic CrB Second-epoch detections are separated by 1.9" and 6.1 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 1369906005476274560 | 15:53:42.59 +32:55:39.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1369906005476274560,2461058.8435,12.21,0.05,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 1369906005476274560 20260118.3435 12.21CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:53:42.19 +32:55:42.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 12.68 15:49:36.77 +34:49:14.8
55.67540 51.36160 galactic CrB Second-epoch detections are separated by 0.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1372546413931606016 | 15:49:37.37 +34:49:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M4V 1995AJ....110.1838R G 179- 57
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1372546413931606016,2461058.8435,12.68,0.05,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
Gaia DR3 1372546413931606016 20260118.3435 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:49:36.77 +34:49:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 13.15 15:53:54.03 +32:50:56.1
52.61780 50.38240 galactic CrB Second-epoch detections are separated by 1.1" and 6.1 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 J238.4772+32.8476 | 15:53:54.03 +32:50:56.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J238.4772+32.8476,2461058.8435,13.15,0.05,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
ATO J238.4772+32.8476 20260118.3435 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:53:54.03 +32:50:56.1 ;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_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.8435,13.43,0.05,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
target 20260118.3435 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:54:50.49 +32:50:16.9 ;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_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 13.53 15:54:32.62 +32:48:26.3
52.56811 50.24463 galactic CrB Second-epoch detections are separated by 2.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J238.6381+32.8061 | 15:54:32.62 +32:48:26.3 (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 J238.6381+32.8061,2461058.8435,13.53,0.05,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
ATO J238.6381+32.8061 20260118.3435 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:54:32.62 +32:48:26.3 ;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_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 11.90 15:48:50.26 +33:57:08.3
54.27579 51.49713 galactic CrB Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1370939993083303936 | 15:48:50.21 +33:57:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.273+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1370939993083303936,2461058.8435,11.90,0.05,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 1370939993083303936 20260118.3435 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-55-53_20.00sec_-14.90C_LIGHT_0655.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:48:50.26 +33:57:08.3 ;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_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 11.65 15:47:14.34 +34:04:29.7
54.45549 51.83233 galactic CrB Second-epoch detections are separated by 0.7" and 6.1 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 1370956245239487232 | 15:47:14.34 +34:04:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.031 (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 1370956245239487232,2461058.8435,11.65,0.05,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
Gaia DR3 1370956245239487232 20260118.3435 11.65CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-55-53_20.00sec_-14.90C_LIGHT_0655.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:47:14.34 +34:04:29.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3435 2461058.8435 11.96 15:53:53.38 +34:12:12.3
54.74017 50.46179 galactic CrB Second-epoch detections are separated by 2.0" 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 J238.4725+34.2033 | 15:53:53.42 +34:12:12.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-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 J238.4725+34.2033,2461058.8435,11.96,0.05,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
ATO J238.4725+34.2033 20260118.3435 11.96CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-54-54_20.00sec_-14.90C_LIGHT_0654.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-05-Q1b1x1_2025-12-23_05-55-53_20.00sec_-14.90C_LIGHT_0655.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-05-Q1b1x1_030241_TTUQ1b1x1_20483_7uEDm4V7/fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20.00sec_-15.00C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:53:53.38 +34:12:12.3 ;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_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-47_20_00sec_-15_00C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-05-Q1b1x1_2025-12-23_05-54-54_20_00sec_-14_90C_LIGHT_0654_fits__*pix.png resample_wcs_fd_Boo-05-Q1b1x1_2026-01-18_02-14-06_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3005 2461058.8005 10.08 20:30:34.02 +65:27:06.2
99.93951 15.05688 galactic Cep Second-epoch detections are separated by 1.2" 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 | Gaia DR3 2246206567973292160 | 20:30:33.18 +65:27:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3 1947AnDea...5....1L DO 38541
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 2246206567973292160,2461058.8005,10.08,0.05,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 2246206567973292160 20260118.3005 10.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-04-Q1b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-12-04_20.00sec_-15.00C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20.00sec_-15.00C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:30:34.02 +65:27:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_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_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3005 2461058.8005 11.87 20:45:03.13 +65:37:06.8
100.96320 13.91934 galactic Cep Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2245696974395332736 | 20:45:01.95 +65:37:04.3 (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 2245696974395332736,2461058.8005,11.87,0.05,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 2245696974395332736 20260118.3005 11.87CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-04-Q1b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-12-04_20.00sec_-15.00C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20.00sec_-15.00C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:45:03.13 +65:37:06.8 ;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-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_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_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3005 2461058.8005 9.43 20:23:20.55 +65:26:45.5
99.51705 15.68715 galactic Dra Second-epoch detections are separated by 0.8" 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 | Gaia DR3 2244745076503100032 | 20:23:20.66 +65:26:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.094+/-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 2244745076503100032,2461058.8005,9.43,0.05,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
Gaia DR3 2244745076503100032 20260118.3005 9.43CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-04-Q1b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-04-Q1b1x1_2025-12-22_20-28-46_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-12-04_20.00sec_-15.00C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20.00sec_-15.00C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:20.55 +65:26:45.5 ;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_Cep-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_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_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3005 2461058.8005 13.13 21:54:17.83 +65:00:58.3
105.59310 8.29219 galactic Cep Second-epoch detections are separated by 8.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2218399334795042176 | 21:54:19.96 +65:01:18.3 (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 2218399334795042176,2461058.8005,13.13,0.05,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
Gaia DR3 2218399334795042176 20260118.3005 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-04-Q1b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-12-04_20.00sec_-15.00C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20.00sec_-15.00C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:17.83 +65:00:58.3 ;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_Cep-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_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_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3005 2461058.8005 12.13 20:16:12.25 +64:37:53.2
98.38837 15.91293 galactic Dra Second-epoch detections are separated by 1.5" 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 | Gaia DR3 2244611073523438720 | 20:16:11.69 +64:37:48.2 (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 2244611073523438720,2461058.8005,12.13,0.05,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 2244611073523438720 20260118.3005 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-04-Q1b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-12-04_20.00sec_-15.00C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cep-04-Q1b1x1_013834_TTUQ1b1x1_17229_McSzvG5z/fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20.00sec_-15.00C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:12.25 +64:37:53.2 ;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_Cep-04-Q1b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q1b1x1_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_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_2026-01-18_01-13-00_20_00sec_-15_00C_LIGHT_0301_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_2026-01-18_01-12-04_20_00sec_-15_00C_LIGHT_0300_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.8972,14.34,0.05,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 20260118.3972 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:21.07 -08:33:51.5 ;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_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.8972,13.55,0.05,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
target 20260118.3972 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:53:41.40 -08:24:55.6 ;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_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3972 2461058.8972 12.80 07:31:27.04 -09:17:54.7
225.79734 4.52448 galactic Mon Second-epoch detections are separated by 6.2" and 9.7 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 J112.8471-09.3084 | 07:31:24.63 -09:18:08.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J112.8471-09.3084,2461058.8972,12.80,0.05,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
ATO J112.8471-09.3084 20260118.3972 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:31:27.04 -09:17:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3972 2461058.8972 13.54 07:14:24.53 -14:58:07.8
228.83999 -1.81921 galactic CMa Second-epoch detections are separated by 1.9" and 9.0 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 3032112053310773376 | 07:14:26.42 -14:58:38.6 (Gaia DR3) | BCEP (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3032112053310773376,2461058.8972,13.54,0.05,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 3032112053310773376 20260118.3972 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:24.53 -14:58:07.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3972 2461058.8972 13.95 07:46:07.27 -06:18:00.9
224.90334 9.15078 galactic Mon Second-epoch detections are separated by 5.3" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | NSVS J0746073-061735 | 07:46:07.46 -06:17:34.4 (Gaia DR3) | L: (local) | 136.000000000000 (local) | Gaia3var=VARIABLE SpType: M8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0746073-061735,2461058.8972,13.95,0.05,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
NSVS J0746073-061735 20260118.3972 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:07.27 -06:18:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.8972,14.12,0.05,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
target 20260118.3972 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:32.74 -14:57:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3972 2461058.8972 14.34 08:08:01.65 -13:55:02.9
234.32587 10.00132 galactic Pup Second-epoch detections are separated by 3.6" 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 5725138186635526912 | 08:08:01.18 -13:55:47.7 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5725138186635526912,2461058.8972,14.34,0.05,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 5725138186635526912 20260118.3972 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:08:01.65 -13:55:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3972 2461058.8972 14.46 07:59:16.98 -10:21:49.9
230.11542 9.98354 galactic Mon Second-epoch detections are separated by 8.9" and 9.8 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 J119.8256-10.3547 | 07:59:18.16 -10:21:17.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J119.8256-10.3547,2461058.8972,14.46,0.05,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
ATO J119.8256-10.3547 20260118.3972 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:59:16.98 -10:21:49.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3972 2461058.8972 14.46 07:58:40.38 -11:01:25.4
230.61745 9.52194 galactic Mon Second-epoch detections are separated by 4.1" and 8.8 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 3036533567515195392 | 07:58:40.08 -11:02:07.4 (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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 3036533567515195392,2461058.8972,14.46,0.05,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
Gaia DR3 3036533567515195392 20260118.3972 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:58:40.38 -11:01:25.4 ;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_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3972 2461058.8972 13.54 07:12:29.58 -05:20:47.0
220.09364 2.22398 galactic Mon Second-epoch detections are separated by 1.9" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.1185-05.3451 | 07:12:29.58 -05:20:47.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.1185-05.3451,2461058.8972,13.54,0.05,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
ATO J108.1185-05.3451 20260118.3972 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20.00sec_-15.00C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Mon-06-Q1b1x1_050406_TTUQ1b1x1_29977_uaa8IlKu/fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:29.58 -05:20:47.0 ;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_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-32-15_20_00sec_-15_00C_LIGHT_0442_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-18_03-31-19_20_00sec_-15_00C_LIGHT_0441_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4191 2461058.9191 13.21 15:18:28.58 +02:07:18.8
3.88748 46.83706 galactic Ser Second-epoch detections are separated by 3.0" 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 | ATO J229.6088+02.1243 | 15:18:28.58 +02:07:18.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4191* 15 18 28.58 +02 07 18.8 13.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J229.6088+02.1243,2461058.9191,13.21,0.05,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
ATO J229.6088+02.1243 20260118.4191 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-05-Q1b1x1_2026-01-09_04-06-36_20.00sec_-15.00C_LIGHT_0083.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-05-Q1b1x1_050007_TTUQ1b1x1_12014_rFP5sgV9/fd_Ser-05-Q1b1x1_2026-01-18_04-03-02_20.00sec_-14.90C_LIGHT_0475.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-05-Q1b1x1_050007_TTUQ1b1x1_12014_rFP5sgV9/fd_Ser-05-Q1b1x1_2026-01-18_04-03-43_20.00sec_-15.00C_LIGHT_0476.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:18:28.58 +02:07:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-05-Q1b1x1_2026-01-09_04-06-36_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png resample_wcs_fd_Ser-05-Q1b1x1_2026-01-18_04-03-43_20_00sec_-15_00C_LIGHT_0476_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-05-Q1b1x1_2026-01-09_04-06-36_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png resample_wcs_fd_Ser-05-Q1b1x1_2026-01-18_04-03-02_20_00sec_-14_90C_LIGHT_0475_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q1b1x1_2026-01-09_04-06-36_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png resample_wcs_fd_Ser-05-Q1b1x1_2026-01-18_04-03-43_20_00sec_-15_00C_LIGHT_0476_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-05-Q1b1x1_2026-01-09_04-06-36_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png resample_wcs_fd_Ser-05-Q1b1x1_2026-01-18_04-03-02_20_00sec_-14_90C_LIGHT_0475_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3891 2461058.8891 11.36 15:56:39.19 +01:53:47.1
11.38127 39.01968 galactic Ser Second-epoch detections are separated by 8.8" and 3.9 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 4411242991398385280 | 15:56:39.59 +01:53:43.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3891* 15 56 39.19 +01 53 47.1 11.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4411242991398385280,2461058.8891,11.36,0.05,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
Gaia DR3 4411242991398385280 20260118.3891 11.36CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-03-Q1b1x1_2026-01-09_03-46-46_20.00sec_-14.90C_LIGHT_0076.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-03-Q1b1x1_044253_TTUQ1b1x1_23002_SGQNcNav/fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20.00sec_-15.00C_LIGHT_0430.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-03-Q1b1x1_044253_TTUQ1b1x1_23002_SGQNcNav/fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20.00sec_-14.90C_LIGHT_0431.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:56:39.19 +01:53:47.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20_00sec_-14_90C_LIGHT_0431_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20_00sec_-15_00C_LIGHT_0430_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20_00sec_-14_90C_LIGHT_0431_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20_00sec_-15_00C_LIGHT_0430_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3891 2461058.8891 11.73 15:56:10.15 +00:56:54.7
10.29021 38.58360 galactic Ser Second-epoch detections are separated by 3.4" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4410845208707857280 | 15:56:10.56 +00:56:50.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3891* 15 56 10.15 +00 56 54.7 11.7 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4410845208707857280,2461058.8891,11.73,0.05,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 4410845208707857280 20260118.3891 11.73CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-03-Q1b1x1_2026-01-09_03-46-46_20.00sec_-14.90C_LIGHT_0076.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-03-Q1b1x1_044253_TTUQ1b1x1_23002_SGQNcNav/fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20.00sec_-15.00C_LIGHT_0430.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-03-Q1b1x1_044253_TTUQ1b1x1_23002_SGQNcNav/fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20.00sec_-14.90C_LIGHT_0431.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:56:10.15 +00:56:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20_00sec_-14_90C_LIGHT_0431_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20_00sec_-15_00C_LIGHT_0430_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20_00sec_-14_90C_LIGHT_0431_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20_00sec_-15_00C_LIGHT_0430_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3891 2461058.8891 12.96 15:55:26.54 +00:56:42.0
10.15370 38.73077 galactic Ser Second-epoch detections are separated by 2.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4410843009684464384 | 15:55:26.91 +00:56:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3891* 15 55 26.54 +00 56 42.0 13.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4410843009684464384,2461058.8891,12.96,0.05,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
Gaia DR3 4410843009684464384 20260118.3891 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-03-Q1b1x1_2026-01-09_03-46-46_20.00sec_-14.90C_LIGHT_0076.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-03-Q1b1x1_044253_TTUQ1b1x1_23002_SGQNcNav/fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20.00sec_-15.00C_LIGHT_0430.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-03-Q1b1x1_044253_TTUQ1b1x1_23002_SGQNcNav/fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20.00sec_-14.90C_LIGHT_0431.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:55:26.54 +00:56:42.0 ;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_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20_00sec_-14_90C_LIGHT_0431_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20_00sec_-15_00C_LIGHT_0430_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20_00sec_-14_90C_LIGHT_0431_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20_00sec_-15_00C_LIGHT_0430_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3891 2461058.8891 13.14 15:56:07.82 +01:19:04.7
10.67256 38.80161 galactic Ser Second-epoch detections are separated by 3.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4411137129044381568 | 15:56:08.21 +01:19:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3891* 15 56 07.82 +01 19 04.7 13.1 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4411137129044381568,2461058.8891,13.14,0.05,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
Gaia DR3 4411137129044381568 20260118.3891 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-03-Q1b1x1_2026-01-09_03-46-46_20.00sec_-14.90C_LIGHT_0076.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-03-Q1b1x1_044253_TTUQ1b1x1_23002_SGQNcNav/fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20.00sec_-15.00C_LIGHT_0430.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-03-Q1b1x1_044253_TTUQ1b1x1_23002_SGQNcNav/fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20.00sec_-14.90C_LIGHT_0431.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:56:07.82 +01:19:04.7 ;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_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20_00sec_-14_90C_LIGHT_0431_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20_00sec_-15_00C_LIGHT_0430_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-20-43_20_00sec_-14_90C_LIGHT_0431_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-03-Q1b1x1_2026-01-09_03-46-46_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png resample_wcs_fd_Ser-03-Q1b1x1_2026-01-18_03-19-34_20_00sec_-15_00C_LIGHT_0430_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4378 2461058.9378 9.80 14:47:45.07 -27:58:56.5
332.08231 28.22472 galactic Hya Second-epoch detections are separated by 0.4" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6219414155609249792 | 14:47:45.06 -27:58:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.042+/-0.039 (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 6219414155609249792,2461058.9378,9.80,0.05,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
Gaia DR3 6219414155609249792 20260118.4378 9.80CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-01-09_04-32-00_20.00sec_-14.90C_LIGHT_0095.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-01-09_04-32-37_20.00sec_-15.00C_LIGHT_0096.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-14-Q1b1x1_053810_TTUQ1b1x1_11432_aTApPaaU/fd_Hya-14-Q1b1x1_2026-01-18_04-29-46_20.00sec_-14.90C_LIGHT_0505.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-14-Q1b1x1_053810_TTUQ1b1x1_11432_aTApPaaU/fd_Hya-14-Q1b1x1_2026-01-18_04-30-39_20.00sec_-14.90C_LIGHT_0506.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:47:45.07 -27:58:56.5 ;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_Hya-14-Q1b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q1b1x1_2026-01-18_04-30-39_20_00sec_-14_90C_LIGHT_0506_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-14-Q1b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q1b1x1_2026-01-18_04-29-46_20_00sec_-14_90C_LIGHT_0505_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-14-Q1b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q1b1x1_2026-01-18_04-30-39_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-14-Q1b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q1b1x1_2026-01-18_04-29-46_20_00sec_-14_90C_LIGHT_0505_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4378 2461058.9378 9.46 14:57:10.01 -27:35:34.5
334.33583 27.50405 galactic Hya Second-epoch detections are separated by 0.1" and 9.6 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 6225267783717101056 | 14:57:10.01 -27:35:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.714+/-0.029 (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 6225267783717101056,2461058.9378,9.46,0.05,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 6225267783717101056 20260118.4378 9.46CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-01-09_04-32-00_20.00sec_-14.90C_LIGHT_0095.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-14-Q1b1x1_2026-01-09_04-32-37_20.00sec_-15.00C_LIGHT_0096.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-14-Q1b1x1_053810_TTUQ1b1x1_11432_aTApPaaU/fd_Hya-14-Q1b1x1_2026-01-18_04-29-46_20.00sec_-14.90C_LIGHT_0505.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Hya-14-Q1b1x1_053810_TTUQ1b1x1_11432_aTApPaaU/fd_Hya-14-Q1b1x1_2026-01-18_04-30-39_20.00sec_-14.90C_LIGHT_0506.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:57:10.01 -27:35:34.5 ;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-14-Q1b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q1b1x1_2026-01-18_04-30-39_20_00sec_-14_90C_LIGHT_0506_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-14-Q1b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q1b1x1_2026-01-18_04-29-46_20_00sec_-14_90C_LIGHT_0505_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-14-Q1b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q1b1x1_2026-01-18_04-30-39_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-14-Q1b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q1b1x1_2026-01-18_04-29-46_20_00sec_-14_90C_LIGHT_0505_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2287 2461058.7287 14.32 07:18:36.95 +01:31:51.7
214.67160 6.74429 galactic CMi Second-epoch detections are separated by 2.3" 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 | target | 07:18:36.95 +01:31:51.7 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.106 (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
target,2461058.7287,14.32,0.05,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
target 20260118.2287 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20.00sec_-15.00C_LIGHT_0216.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20.00sec_-15.00C_LIGHT_0217.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:18:36.95 +01:31:51.7 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.7287,14.49,0.05,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
target 20260118.2287 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20.00sec_-15.00C_LIGHT_0216.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20.00sec_-15.00C_LIGHT_0217.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:02.40 +02:01:36.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2287 2461058.7287 12.86 08:10:29.88 +10:02:11.5
212.72997 22.07517 galactic Cnc Second-epoch detections are separated by 0.7" 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 | target | 08:10:29.88 +10:02:11.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.313+/-0.029 (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,2461058.7287,12.86,0.05,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
target 20260118.2287 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-43_20.00sec_-15.00C_LIGHT_0450.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20.00sec_-15.00C_LIGHT_0216.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20.00sec_-15.00C_LIGHT_0217.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:29.88 +10:02:11.5 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2287 2461058.7287 13.12 08:13:52.29 +05:27:59.2
217.53296 20.81003 galactic Hya Second-epoch detections are separated by 1.5" 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 3096322295411224448 | 08:13:50.31 +05:27:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.290+/-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 3096322295411224448,2461058.7287,13.12,0.05,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 3096322295411224448 20260118.2287 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-43_20.00sec_-15.00C_LIGHT_0450.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20.00sec_-15.00C_LIGHT_0216.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20.00sec_-15.00C_LIGHT_0217.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:52.29 +05:27:59.2 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2287 2461058.7287 13.19 08:11:10.45 +07:19:45.3
215.42860 21.04630 galactic Cnc Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:11:10.45 +07:19:45.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.513+/-0.035 (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,2461058.7287,13.19,0.05,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
target 20260118.2287 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-43_20.00sec_-15.00C_LIGHT_0450.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20.00sec_-15.00C_LIGHT_0216.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20.00sec_-15.00C_LIGHT_0217.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:10.45 +07:19:45.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2287 2461058.7287 12.19 08:10:43.93 +10:44:04.1
212.07418 22.42452 galactic Cnc Second-epoch detections are separated by 0.1" 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 648878062740205056 | 08:10:43.93 +10:44:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5) J-Ks=0.205+/-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 648878062740205056,2461058.7287,12.19,0.05,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
Gaia DR3 648878062740205056 20260118.2287 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 /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMi-01-Q1b1x1_2025-12-23_02-47-43_20.00sec_-15.00C_LIGHT_0450.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20.00sec_-15.00C_LIGHT_0216.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CMi-01-Q1b1x1_042410_TTUQ1b1x1_5561_ZCVDVfeb/fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20.00sec_-15.00C_LIGHT_0217.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:43.93 +10:44:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-29-35_20_00sec_-15_00C_LIGHT_0217_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-17_23-28-45_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4038 2461058.9038 12.80 16:32:10.52 +08:58:10.7
24.62566 34.96017 galactic Her Second-epoch detections are separated by 3.8" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4440454369650191744 | 16:32:11.38 +08:58:02.0 (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 01 18.4037* 16 32 10.52 +08 58 10.7 12.8 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 4440454369650191744,2461058.9038,12.80,0.05,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
Gaia DR3 4440454369650191744 20260118.4038 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-02-Q1b1x1_2026-01-09_03-58-24_20.00sec_-14.90C_LIGHT_0079.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20.00sec_-14.90C_LIGHT_0451.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20.00sec_-15.00C_LIGHT_0452.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:32:10.52 +08:58:10.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4038 2461058.9038 12.71 16:32:10.49 +08:56:30.8
24.59541 34.94771 galactic Her Second-epoch detections are separated by 3.1" and 9.0 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 4440454262270461056 | 16:32:11.35 +08:56:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4037* 16 32 10.49 +08 56 30.8 12.7 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 4440454262270461056,2461058.9038,12.71,0.05,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
Gaia DR3 4440454262270461056 20260118.4038 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-02-Q1b1x1_2026-01-09_03-58-24_20.00sec_-14.90C_LIGHT_0079.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20.00sec_-14.90C_LIGHT_0451.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20.00sec_-15.00C_LIGHT_0452.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:32:10.49 +08:56:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4038 2461058.9038 13.20 16:31:37.59 +08:51:29.4
24.42933 35.03041 galactic Her Second-epoch detections are separated by 5.0" and 8.7 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 4440447428978409600 | 16:31:38.46 +08:51:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4037* 16 31 37.59 +08 51 29.4 13.2 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 4440447428978409600,2461058.9038,13.20,0.05,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
Gaia DR3 4440447428978409600 20260118.4038 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-02-Q1b1x1_2026-01-09_03-58-24_20.00sec_-14.90C_LIGHT_0079.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20.00sec_-14.90C_LIGHT_0451.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20.00sec_-15.00C_LIGHT_0452.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:31:37.59 +08:51:29.4 ;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_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4038 2461058.9038 13.64 16:06:18.50 +11:06:15.0
23.40103 41.60678 galactic Ser Second-epoch detections are separated by 1.1" and 9.1 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 4456757275226448128 | 16:06:20.72 +11:05:52.8 (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 01 18.4037* 16 06 18.50 +11 06 15.0 13.6 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4456757275226448128,2461058.9038,13.64,0.05,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 4456757275226448128 20260118.4038 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-02-Q1b1x1_2026-01-09_03-58-24_20.00sec_-14.90C_LIGHT_0079.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20.00sec_-14.90C_LIGHT_0451.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20.00sec_-15.00C_LIGHT_0452.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:06:18.50 +11:06:15.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4038 2461058.9038 13.69 16:16:08.44 +09:38:46.0
23.12936 38.79098 galactic Her Second-epoch detections are separated by 6.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 16:16:08.44 +09:38:46.0 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4037* 16 16 08.44 +09 38 46.0 13.7 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
target,2461058.9038,13.69,0.05,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
target 20260118.4038 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-02-Q1b1x1_2026-01-09_03-58-24_20.00sec_-14.90C_LIGHT_0079.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20.00sec_-14.90C_LIGHT_0451.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-02-Q1b1x1_042216_TTUQ1b1x1_14641_OL671OEs/fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20.00sec_-15.00C_LIGHT_0452.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:16:08.44 +09:38:46.0 ;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_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-41-39_20_00sec_-15_00C_LIGHT_0452_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q1b1x1_2026-01-09_03-58-24_20_00sec_-14_90C_LIGHT_0079_fits__*pix.png resample_wcs_fd_Ser-02-Q1b1x1_2026-01-18_03-40-48_20_00sec_-14_90C_LIGHT_0451_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4640 2461058.9640 12.19 15:53:10.98 -30:59:33.2
342.75062 17.49065 galactic Lup 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 | ATO J238.2901-31.0000 | 15:53:11.36 -30:59:38.6 (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 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 J238.2901-31.0000,2461058.9640,12.19,0.05,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
ATO J238.2901-31.0000 20260118.4640 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lib-05-Q1b1x1_2026-01-09_05-30-49_20.00sec_-14.90C_LIGHT_0121.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-05-Q1b1x1_054011_TTUQ1b1x1_16474_x6MleoGe/fd_Lib-05-Q1b1x1_2026-01-18_05-07-30_20.00sec_-15.00C_LIGHT_0521.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-05-Q1b1x1_054011_TTUQ1b1x1_16474_x6MleoGe/fd_Lib-05-Q1b1x1_2026-01-18_05-08-20_20.00sec_-15.00C_LIGHT_0522.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:53:10.98 -30:59:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-05-Q1b1x1_2026-01-09_05-30-49_20_00sec_-14_90C_LIGHT_0121_fits__*pix.png resample_wcs_fd_Lib-05-Q1b1x1_2026-01-18_05-08-20_20_00sec_-15_00C_LIGHT_0522_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-05-Q1b1x1_2026-01-09_05-30-49_20_00sec_-14_90C_LIGHT_0121_fits__*pix.png resample_wcs_fd_Lib-05-Q1b1x1_2026-01-18_05-07-30_20_00sec_-15_00C_LIGHT_0521_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-05-Q1b1x1_2026-01-09_05-30-49_20_00sec_-14_90C_LIGHT_0121_fits__*pix.png resample_wcs_fd_Lib-05-Q1b1x1_2026-01-18_05-08-20_20_00sec_-15_00C_LIGHT_0522_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-05-Q1b1x1_2026-01-09_05-30-49_20_00sec_-14_90C_LIGHT_0121_fits__*pix.png resample_wcs_fd_Lib-05-Q1b1x1_2026-01-18_05-07-30_20_00sec_-15_00C_LIGHT_0521_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4640 2461058.9640 12.69 15:53:08.02 -30:55:46.3
342.78628 17.54476 galactic Lup Second-epoch detections are separated by 1.2" 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 6039744949086903936 | 15:53:08.33 -30:55:51.0 (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 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 6039744949086903936,2461058.9640,12.69,0.05,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
Gaia DR3 6039744949086903936 20260118.4640 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lib-05-Q1b1x1_2026-01-09_05-30-49_20.00sec_-14.90C_LIGHT_0121.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-05-Q1b1x1_054011_TTUQ1b1x1_16474_x6MleoGe/fd_Lib-05-Q1b1x1_2026-01-18_05-07-30_20.00sec_-15.00C_LIGHT_0521.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-05-Q1b1x1_054011_TTUQ1b1x1_16474_x6MleoGe/fd_Lib-05-Q1b1x1_2026-01-18_05-08-20_20.00sec_-15.00C_LIGHT_0522.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:53:08.02 -30:55:46.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-05-Q1b1x1_2026-01-09_05-30-49_20_00sec_-14_90C_LIGHT_0121_fits__*pix.png resample_wcs_fd_Lib-05-Q1b1x1_2026-01-18_05-08-20_20_00sec_-15_00C_LIGHT_0522_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-05-Q1b1x1_2026-01-09_05-30-49_20_00sec_-14_90C_LIGHT_0121_fits__*pix.png resample_wcs_fd_Lib-05-Q1b1x1_2026-01-18_05-07-30_20_00sec_-15_00C_LIGHT_0521_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-05-Q1b1x1_2026-01-09_05-30-49_20_00sec_-14_90C_LIGHT_0121_fits__*pix.png resample_wcs_fd_Lib-05-Q1b1x1_2026-01-18_05-08-20_20_00sec_-15_00C_LIGHT_0522_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-05-Q1b1x1_2026-01-09_05-30-49_20_00sec_-14_90C_LIGHT_0121_fits__*pix.png resample_wcs_fd_Lib-05-Q1b1x1_2026-01-18_05-07-30_20_00sec_-15_00C_LIGHT_0521_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.7586,13.97,0.05,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
target 20260118.2586 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cnc-05-Q1b1x1_040636_TTUQ1b1x1_3915_Ifdut76h/fd_Cnc-05-Q1b1x1_2026-01-18_00-11-48_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cnc-05-Q1b1x1_040636_TTUQ1b1x1_3915_Ifdut76h/fd_Cnc-05-Q1b1x1_2026-01-18_00-12-37_20.00sec_-14.90C_LIGHT_0260.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:36.23 +16:36:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-18_00-12-37_20_00sec_-14_90C_LIGHT_0260_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-18_00-11-48_20_00sec_-15_00C_LIGHT_0259_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-18_00-12-37_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-18_00-11-48_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2586 2461058.7586 14.14 08:34:12.75 +09:45:19.6
215.77052 27.22888 galactic Cnc Second-epoch detections are separated by 7.4" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 599793905169558784 | 08:34:10.99 +09:45:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 599793905169558784,2461058.7586,14.14,0.05,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 599793905169558784 20260118.2586 14.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cnc-05-Q1b1x1_040636_TTUQ1b1x1_3915_Ifdut76h/fd_Cnc-05-Q1b1x1_2026-01-18_00-11-48_20.00sec_-15.00C_LIGHT_0259.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cnc-05-Q1b1x1_040636_TTUQ1b1x1_3915_Ifdut76h/fd_Cnc-05-Q1b1x1_2026-01-18_00-12-37_20.00sec_-14.90C_LIGHT_0260.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:34:12.75 +09:45:19.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-18_00-12-37_20_00sec_-14_90C_LIGHT_0260_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-18_00-11-48_20_00sec_-15_00C_LIGHT_0259_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-18_00-12-37_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-18_00-11-48_20_00sec_-15_00C_LIGHT_0259_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4701 2461058.9701 11.51 15:16:13.29 -38:57:23.2
331.43402 15.77241 galactic Lup Second-epoch detections are separated by 0.6" 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 | Gaia DR3 6006806677394576768 | 15:16:13.76 -38:57:28.3 (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 6006806677394576768,2461058.9701,11.51,0.05,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
Gaia DR3 6006806677394576768 20260118.4701 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cen-03-Q1b1x1_2026-01-09_05-36-16_20.00sec_-15.00C_LIGHT_0127.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cen-03-Q1b1x1_054818_TTUQ1b1x1_15253_dSaeRXRP/fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20.00sec_-15.00C_LIGHT_0529.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cen-03-Q1b1x1_054818_TTUQ1b1x1_15253_dSaeRXRP/fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20.00sec_-15.00C_LIGHT_0530.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:16:13.29 -38:57:23.2 ;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_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20_00sec_-15_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20_00sec_-15_00C_LIGHT_0529_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20_00sec_-15_00C_LIGHT_0530_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20_00sec_-15_00C_LIGHT_0529_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4701 2461058.9701 11.67 15:16:04.26 -38:56:30.8
331.41680 15.80058 galactic Lup Second-epoch detections are separated by 1.9" 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 | Gaia DR3 6006807673827005568 | 15:16:04.62 -38:56:35.7 (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 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 6006807673827005568,2461058.9701,11.67,0.05,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 6006807673827005568 20260118.4701 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cen-03-Q1b1x1_2026-01-09_05-36-16_20.00sec_-15.00C_LIGHT_0127.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cen-03-Q1b1x1_054818_TTUQ1b1x1_15253_dSaeRXRP/fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20.00sec_-15.00C_LIGHT_0529.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cen-03-Q1b1x1_054818_TTUQ1b1x1_15253_dSaeRXRP/fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20.00sec_-15.00C_LIGHT_0530.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:16:04.26 -38:56:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20_00sec_-15_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20_00sec_-15_00C_LIGHT_0529_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20_00sec_-15_00C_LIGHT_0530_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20_00sec_-15_00C_LIGHT_0529_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4701 2461058.9701 12.01 15:15:57.93 -38:57:14.8
331.39200 15.80153 galactic Lup Second-epoch detections are separated by 1.8" 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 | Gaia DR3 6006807261510144256 | 15:15:58.30 -38:57:19.7 (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 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 6006807261510144256,2461058.9701,12.01,0.05,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
Gaia DR3 6006807261510144256 20260118.4701 12.01CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cen-03-Q1b1x1_2026-01-09_05-36-16_20.00sec_-15.00C_LIGHT_0127.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cen-03-Q1b1x1_054818_TTUQ1b1x1_15253_dSaeRXRP/fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20.00sec_-15.00C_LIGHT_0529.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cen-03-Q1b1x1_054818_TTUQ1b1x1_15253_dSaeRXRP/fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20.00sec_-15.00C_LIGHT_0530.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:15:57.93 -38:57:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20_00sec_-15_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20_00sec_-15_00C_LIGHT_0529_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20_00sec_-15_00C_LIGHT_0530_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20_00sec_-15_00C_LIGHT_0529_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4701 2461058.9701 12.07 15:15:50.95 -39:01:25.0
331.33294 15.75559 galactic Lup Second-epoch detections are separated by 1.0" 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 | Gaia DR3 6006805401780102400 | 15:15:51.39 -39:01:30.0 (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 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 6006805401780102400,2461058.9701,12.07,0.05,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
Gaia DR3 6006805401780102400 20260118.4701 12.07CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cen-03-Q1b1x1_2026-01-09_05-36-16_20.00sec_-15.00C_LIGHT_0127.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cen-03-Q1b1x1_054818_TTUQ1b1x1_15253_dSaeRXRP/fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20.00sec_-15.00C_LIGHT_0529.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cen-03-Q1b1x1_054818_TTUQ1b1x1_15253_dSaeRXRP/fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20.00sec_-15.00C_LIGHT_0530.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:15:50.95 -39:01:25.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20_00sec_-15_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20_00sec_-15_00C_LIGHT_0529_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-17-19_20_00sec_-15_00C_LIGHT_0530_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-03-Q1b1x1_2026-01-09_05-36-16_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_Cen-03-Q1b1x1_2026-01-18_05-16-12_20_00sec_-15_00C_LIGHT_0529_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4402 2461058.9402 10.69 16:48:22.44 -05:52:02.9
12.23060 23.97003 galactic Oph Second-epoch detections are separated by 0.8" and 9.6 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 4341287216915136512 | 16:48:22.11 -05:51:59.4 (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 4341287216915136512,2461058.9402,10.69,0.05,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
Gaia DR3 4341287216915136512 20260118.4402 10.69CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-06-Q1b1x1_2026-01-09_04-57-40_20.00sec_-14.90C_LIGHT_0105.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20.00sec_-15.00C_LIGHT_0509.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20.00sec_-15.00C_LIGHT_0510.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:48:22.44 -05:52:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4402 2461058.9402 10.92 16:48:24.78 -05:14:36.1
12.80954 24.30242 galactic Oph Second-epoch detections are separated by 1.7" and 9.4 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 4353356934011333248 | 16:48:25.16 -05:14:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4353356934011333248,2461058.9402,10.92,0.05,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 4353356934011333248 20260118.4402 10.92CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-06-Q1b1x1_2026-01-09_04-57-40_20.00sec_-14.90C_LIGHT_0105.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20.00sec_-15.00C_LIGHT_0509.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20.00sec_-15.00C_LIGHT_0510.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:48:24.78 -05:14:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4402 2461058.9402 12.31 16:48:24.68 -05:20:10.8
12.72372 24.25218 galactic Oph Second-epoch detections are separated by 0.9" and 9.5 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 J252.0974-05.3281 | 16:48:25.08 -05:20:12.1 (Gaia DR3) | STOCH (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 J252.0974-05.3281,2461058.9402,12.31,0.05,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
ATO J252.0974-05.3281 20260118.4402 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-06-Q1b1x1_2026-01-09_04-57-40_20.00sec_-14.90C_LIGHT_0105.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20.00sec_-15.00C_LIGHT_0509.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20.00sec_-15.00C_LIGHT_0510.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:48:24.68 -05:20:10.8 ;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_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4402 2461058.9402 12.69 16:48:48.54 -05:11:40.9
12.91313 24.24611 galactic Oph Second-epoch detections are separated by 1.5" and 9.7 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 4353356830931029120 | 16:48:48.99 -05:11:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4353356830931029120,2461058.9402,12.69,0.05,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
Gaia DR3 4353356830931029120 20260118.4402 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-06-Q1b1x1_2026-01-09_04-57-40_20.00sec_-14.90C_LIGHT_0105.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20.00sec_-15.00C_LIGHT_0509.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20.00sec_-15.00C_LIGHT_0510.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:48:48.54 -05:11:40.9 ;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_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4402 2461058.9402 13.05 16:48:25.30 -05:45:00.0
12.34534 24.02436 galactic Oph Second-epoch detections are separated by 1.8" and 9.8 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 4341292783194242944 | 16:48:24.88 -05:44:56.8 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4341292783194242944,2461058.9402,13.05,0.05,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 4341292783194242944 20260118.4402 13.05CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-06-Q1b1x1_2026-01-09_04-57-40_20.00sec_-14.90C_LIGHT_0105.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20.00sec_-15.00C_LIGHT_0509.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20.00sec_-15.00C_LIGHT_0510.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:48:25.30 -05:45:00.0 ;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_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.9402,13.44,0.05,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
target 20260118.4402 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-06-Q1b1x1_2026-01-09_04-57-40_20.00sec_-14.90C_LIGHT_0105.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20.00sec_-15.00C_LIGHT_0509.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20.00sec_-15.00C_LIGHT_0510.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:33:17.54 -01:37:45.9 ;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_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4402 2461058.9402 10.83 16:36:38.32 -06:29:18.0
9.86938 26.04731 galactic Oph Second-epoch detections are separated by 1.8" and 9.6 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 4351528446172568448 | 16:36:38.27 -06:29:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.783+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4351528446172568448,2461058.9402,10.83,0.05,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
Gaia DR3 4351528446172568448 20260118.4402 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-06-Q1b1x1_2026-01-09_04-57-40_20.00sec_-14.90C_LIGHT_0105.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Ser-06-Q1b1x1_2026-01-09_04-58-37_20.00sec_-15.00C_LIGHT_0106.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20.00sec_-15.00C_LIGHT_0509.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Ser-06-Q1b1x1_050209_TTUQ1b1x1_12427_UZKefDVu/fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20.00sec_-15.00C_LIGHT_0510.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:36:38.32 -06:29:18.0 ;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_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-34-08_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-06-Q1b1x1_2026-01-09_04-57-40_20_00sec_-14_90C_LIGHT_0105_fits__*pix.png resample_wcs_fd_Ser-06-Q1b1x1_2026-01-18_04-33-24_20_00sec_-15_00C_LIGHT_0509_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4336 2461058.9336 11.47 15:38:02.20 -21:19:24.4
346.93418 26.98021 galactic Lib Second-epoch detections are separated by 0.2" 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 | Gaia DR3 6241382604091945856 | 15:38:02.24 -21:19:18.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 1985ApJS...59..197B LHS 3097
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 6241382604091945856,2461058.9336,11.47,0.05,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
Gaia DR3 6241382604091945856 20260118.4336 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-01-09_04-39-36_20.00sec_-15.00C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20.00sec_-15.00C_LIGHT_0499.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20.00sec_-15.00C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:38:02.20 -21:19:24.4 ;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_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4336 2461058.9336 13.10 15:38:20.58 -22:32:11.9
346.09705 26.02331 galactic Lib Second-epoch detections are separated by 1.2" 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 6240962551993233152 | 15:38:20.24 -22:32:08.2 (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 6240962551993233152,2461058.9336,13.10,0.05,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
Gaia DR3 6240962551993233152 20260118.4336 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-01-09_04-39-36_20.00sec_-15.00C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20.00sec_-15.00C_LIGHT_0499.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20.00sec_-15.00C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:38:20.58 -22:32:11.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4336 2461058.9336 13.28 15:38:07.38 -22:26:12.0
346.12786 26.13199 galactic Lib Second-epoch detections are separated by 2.1" 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 J234.5292-22.4357 | 15:38:07.38 -22:26:12.0 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J234.5292-22.4357,2461058.9336,13.28,0.05,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
ATO J234.5292-22.4357 20260118.4336 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-01-09_04-39-36_20.00sec_-15.00C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20.00sec_-15.00C_LIGHT_0499.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20.00sec_-15.00C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:38:07.38 -22:26:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4336 2461058.9336 13.43 14:47:25.73 -13:42:57.4
341.13191 40.39870 galactic Lib Second-epoch detections are separated by 4.6" 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 | target | 14:47:25.73 -13:42:57.4 (user input) | T | P | (position from user input) J-Ks=1.001+/-0.131 (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
target,2461058.9336,13.43,0.05,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
target 20260118.4336 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-01-09_04-39-36_20.00sec_-15.00C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20.00sec_-15.00C_LIGHT_0499.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20.00sec_-15.00C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:47:25.73 -13:42:57.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4336 2461058.9336 13.41 14:47:28.39 -22:16:40.7
335.35772 33.18696 galactic Lib Second-epoch detections are separated by 1.7" and 6.3 pix This object is listed in tocp_transients_list.txt 3.5" PSN J14472863-2216396 2011-05-10.23 15.5mag
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6278757370844404224 | 14:47:28.39 -22:16:40.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.167+/-0.076 (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
Large-amplitude variable Gaia DR2 6278757370844404224,2461058.9336,13.41,0.05,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
Large-amplitude variable Gaia DR2 6278757370844404224 20260118.4336 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-01-09_04-39-36_20.00sec_-15.00C_LIGHT_0099.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20.00sec_-15.00C_LIGHT_0499.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-03-Q1b1x1_052812_TTUQ1b1x1_13988_QAnT1XIJ/fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20.00sec_-15.00C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:47:28.39 -22:16:40.7 ;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_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-24-34_20_00sec_-15_00C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q1b1x1_2026-01-09_04-39-36_20_00sec_-15_00C_LIGHT_0099_fits__*pix.png resample_wcs_fd_Lib-03-Q1b1x1_2026-01-18_04-23-44_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.8986,11.73,0.05,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
target 20260118.3986 11.73CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_060016_TTUQ1b1x1_25340_HEONV9OR/fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20.00sec_-14.90C_LIGHT_0443.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_060016_TTUQ1b1x1_25340_HEONV9OR/fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20.00sec_-15.00C_LIGHT_0444.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:19.99 +51:03:11.4 ;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_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20_00sec_-15_00C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20_00sec_-14_90C_LIGHT_0443_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20_00sec_-15_00C_LIGHT_0444_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20_00sec_-14_90C_LIGHT_0443_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3986 2461058.8986 12.28 09:12:38.09 +56:32:38.5
159.92372 41.60185 galactic UMa Second-epoch detections are separated by 6.1" and 4.0 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 1024517551713963648 | 09:12:37.51 +56:32:46.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3986* 09 12 38.09 +56 32 38.5 12.3 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
Gaia DR3 1024517551713963648,2461058.8986,12.28,0.05,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
Gaia DR3 1024517551713963648 20260118.3986 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_060016_TTUQ1b1x1_25340_HEONV9OR/fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20.00sec_-14.90C_LIGHT_0443.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_060016_TTUQ1b1x1_25340_HEONV9OR/fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20.00sec_-15.00C_LIGHT_0444.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:38.09 +56:32:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20_00sec_-15_00C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20_00sec_-14_90C_LIGHT_0443_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20_00sec_-15_00C_LIGHT_0444_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20_00sec_-14_90C_LIGHT_0443_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.8986,13.67,0.05,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 20260118.3986 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_060016_TTUQ1b1x1_25340_HEONV9OR/fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20.00sec_-14.90C_LIGHT_0443.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_060016_TTUQ1b1x1_25340_HEONV9OR/fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20.00sec_-15.00C_LIGHT_0444.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:48:00.44 +48:58:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20_00sec_-15_00C_LIGHT_0444_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20_00sec_-14_90C_LIGHT_0443_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-34-08_20_00sec_-15_00C_LIGHT_0444_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_03-33-30_20_00sec_-14_90C_LIGHT_0443_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4025 2461058.9025 10.68 19:52:44.69 +56:41:57.2
89.75958 14.59317 galactic Cyg Second-epoch detections are separated by 2.1" and 6.8 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 J298.1971+56.7041 | 19:52:45.10 +56:41:52.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.1971+56.7041,2461058.9025,10.68,0.05,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
ATO J298.1971+56.7041 20260118.4025 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-08-Q1b1x1_2026-01-09_03-33-26_20.00sec_-15.00C_LIGHT_0062.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-08-Q1b1x1_055821_TTUQ1b1x1_25961_wKkybjcQ/fd_Dra-08-Q1b1x1_2026-01-18_03-39-00_20.00sec_-15.00C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-08-Q1b1x1_055821_TTUQ1b1x1_25961_wKkybjcQ/fd_Dra-08-Q1b1x1_2026-01-18_03-39-55_20.00sec_-15.00C_LIGHT_0450.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:44.69 +56:41:57.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-08-Q1b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q1b1x1_2026-01-18_03-39-55_20_00sec_-15_00C_LIGHT_0450_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-08-Q1b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q1b1x1_2026-01-18_03-39-00_20_00sec_-15_00C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-08-Q1b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q1b1x1_2026-01-18_03-39-55_20_00sec_-15_00C_LIGHT_0450_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-08-Q1b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q1b1x1_2026-01-18_03-39-00_20_00sec_-15_00C_LIGHT_0449_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3943 2461058.8943 14.02 16:59:26.45 +49:55:19.3
76.62801 38.16336 galactic Her Second-epoch detections are separated by 3.7" 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 | target | 16:59:26.45 +49:55:19.3 (user input) | T | P | (position from user input) J-Ks=0.941+/-0.128 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3943* 16 59 26.45 +49 55 19.3 14.0 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
target,2461058.8943,14.02,0.05,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
target 20260118.3943 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-10-Q1b1x1_2026-01-09_03-16-10_20.00sec_-15.00C_LIGHT_0044.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-10-Q1b1x1_060203_TTUQ1b1x1_32477_bZCTOHeQ/fd_Dra-10-Q1b1x1_2026-01-18_03-27-16_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-10-Q1b1x1_060203_TTUQ1b1x1_32477_bZCTOHeQ/fd_Dra-10-Q1b1x1_2026-01-18_03-28-01_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:59:26.45 +49:55:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-10-Q1b1x1_2026-01-09_03-16-10_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Dra-10-Q1b1x1_2026-01-18_03-28-01_20_00sec_-15_00C_LIGHT_0438_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_2026-01-18_03-27-16_20_00sec_-15_00C_LIGHT_0437_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_2026-01-18_03-28-01_20_00sec_-15_00C_LIGHT_0438_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_2026-01-18_03-27-16_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3943 2461058.8943 8.36 17:45:57.89 +49:31:06.2
76.54844 30.64073 galactic Her Second-epoch detections are separated by 0.6" 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 1364025542413184768 | 17:45:57.95 +49:31:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.612+/-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!
TCP 2026 01 18.3943* 17 45 57.89 +49 31 06.2 8.4 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 1364025542413184768,2461058.8943,8.36,0.05,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
Gaia DR3 1364025542413184768 20260118.3943 8.36CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-10-Q1b1x1_2026-01-09_03-16-10_20.00sec_-15.00C_LIGHT_0044.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-10-Q1b1x1_2026-01-09_03-16-57_20.00sec_-14.90C_LIGHT_0045.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-10-Q1b1x1_060203_TTUQ1b1x1_32477_bZCTOHeQ/fd_Dra-10-Q1b1x1_2026-01-18_03-27-16_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-10-Q1b1x1_060203_TTUQ1b1x1_32477_bZCTOHeQ/fd_Dra-10-Q1b1x1_2026-01-18_03-28-01_20.00sec_-15.00C_LIGHT_0438.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:45:57.89 +49:31:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-10-Q1b1x1_2026-01-09_03-16-10_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Dra-10-Q1b1x1_2026-01-18_03-28-01_20_00sec_-15_00C_LIGHT_0438_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_2026-01-18_03-27-16_20_00sec_-15_00C_LIGHT_0437_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_2026-01-18_03-28-01_20_00sec_-15_00C_LIGHT_0438_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_2026-01-18_03-27-16_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4663 2461058.9663 10.12 20:34:33.05 +48:42:49.2
86.31696 5.00568 galactic Cyg Second-epoch detections are separated by 0.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J308.6311+48.7077 | 20:34:33.61 +48:42:44.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 1952CoRut..32....1H BD+48 3165
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 J308.6311+48.7077,2461058.9663,10.12,0.05,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 J308.6311+48.7077 20260118.4663 10.12CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-01-Q1b1x1_2026-01-09_05-29-02_20.00sec_-14.90C_LIGHT_0119.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cyg-01-Q1b1x1_060607_TTUQ1b1x1_8985_96jb3YhN/fd_Cyg-01-Q1b1x1_2026-01-18_05-10-52_20.00sec_-15.00C_LIGHT_0525.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cyg-01-Q1b1x1_060607_TTUQ1b1x1_8985_96jb3YhN/fd_Cyg-01-Q1b1x1_2026-01-18_05-11-43_20.00sec_-14.90C_LIGHT_0526.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:34:33.05 +48:42:49.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-18_05-11-43_20_00sec_-14_90C_LIGHT_0526_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-18_05-10-52_20_00sec_-15_00C_LIGHT_0525_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-18_05-11-43_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-18_05-10-52_20_00sec_-15_00C_LIGHT_0525_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4663 2461058.9663 10.92 20:35:49.34 +48:48:00.3
86.51191 4.88879 galactic Cyg Second-epoch detections are separated by 4.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2179781634575880192 | 20:35:50.03 +48:47:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2179781634575880192,2461058.9663,10.92,0.05,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 2179781634575880192 20260118.4663 10.92CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-01-Q1b1x1_2026-01-09_05-29-02_20.00sec_-14.90C_LIGHT_0119.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cyg-01-Q1b1x1_060607_TTUQ1b1x1_8985_96jb3YhN/fd_Cyg-01-Q1b1x1_2026-01-18_05-10-52_20.00sec_-15.00C_LIGHT_0525.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Cyg-01-Q1b1x1_060607_TTUQ1b1x1_8985_96jb3YhN/fd_Cyg-01-Q1b1x1_2026-01-18_05-11-43_20.00sec_-14.90C_LIGHT_0526.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:35:49.34 +48:48:00.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-18_05-11-43_20_00sec_-14_90C_LIGHT_0526_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-18_05-10-52_20_00sec_-15_00C_LIGHT_0525_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-18_05-11-43_20_00sec_-14_90C_LIGHT_0526_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-18_05-10-52_20_00sec_-15_00C_LIGHT_0525_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4674 2461058.9674 10.13 19:55:10.74 +40:49:17.5
75.84609 6.49804 galactic Cyg Second-epoch detections are separated by 1.3" and 8.8 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 J298.7844+40.8247 | 19:55:11.47 +40:49:11.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9.5IV/V 2016AJ....151...13G LAMOST J195511.47+404911.6
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 J298.7844+40.8247,2461058.9674,10.13,0.05,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 J298.7844+40.8247 20260118.4674 10.13CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyr-01-Q1b1x1_2026-01-09_05-34-22_20.00sec_-15.00C_LIGHT_0125.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyr-01-Q1b1x1_061206_TTUQ1b1x1_12279_s6RAOhWT/fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20.00sec_-15.00C_LIGHT_0527.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyr-01-Q1b1x1_061206_TTUQ1b1x1_12279_s6RAOhWT/fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20.00sec_-14.90C_LIGHT_0528.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:10.74 +40:49:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20_00sec_-14_90C_LIGHT_0528_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20_00sec_-15_00C_LIGHT_0527_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20_00sec_-14_90C_LIGHT_0528_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20_00sec_-15_00C_LIGHT_0527_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4674 2461058.9674 11.25 19:55:12.04 +41:02:45.2
76.04272 6.60847 galactic Cyg Second-epoch detections are separated by 1.3" and 8.7 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 2075315282476810112 | 19:55:12.66 +41:02:41.6 (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 2075315282476810112,2461058.9674,11.25,0.05,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
Gaia DR3 2075315282476810112 20260118.4674 11.25CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyr-01-Q1b1x1_2026-01-09_05-34-22_20.00sec_-15.00C_LIGHT_0125.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyr-01-Q1b1x1_061206_TTUQ1b1x1_12279_s6RAOhWT/fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20.00sec_-15.00C_LIGHT_0527.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyr-01-Q1b1x1_061206_TTUQ1b1x1_12279_s6RAOhWT/fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20.00sec_-14.90C_LIGHT_0528.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:12.04 +41:02:45.2 ;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_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20_00sec_-14_90C_LIGHT_0528_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20_00sec_-15_00C_LIGHT_0527_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20_00sec_-14_90C_LIGHT_0528_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20_00sec_-15_00C_LIGHT_0527_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4674 2461058.9674 11.24 19:55:22.68 +41:14:14.2
76.22578 6.67690 galactic Cyg Second-epoch detections are separated by 1.1" and 8.7 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 J298.8376+41.2445 | 19:55:23.18 +41:14:11.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1925AnHar.100....1C HD 226569
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 J298.8376+41.2445,2461058.9674,11.24,0.05,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
ATO J298.8376+41.2445 20260118.4674 11.24CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyr-01-Q1b1x1_2026-01-09_05-34-22_20.00sec_-15.00C_LIGHT_0125.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyr-01-Q1b1x1_061206_TTUQ1b1x1_12279_s6RAOhWT/fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20.00sec_-15.00C_LIGHT_0527.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyr-01-Q1b1x1_061206_TTUQ1b1x1_12279_s6RAOhWT/fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20.00sec_-14.90C_LIGHT_0528.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:55:22.68 +41:14:14.2 ;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_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20_00sec_-14_90C_LIGHT_0528_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20_00sec_-15_00C_LIGHT_0527_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-13-21_20_00sec_-14_90C_LIGHT_0528_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-01-Q1b1x1_2026-01-09_05-34-22_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png resample_wcs_fd_Lyr-01-Q1b1x1_2026-01-18_05-12-30_20_00sec_-15_00C_LIGHT_0527_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4080 2461058.9080 10.34 19:08:33.88 +52:07:38.0
82.69281 18.61155 galactic Cyg Second-epoch detections are separated by 0.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2134205739425084288 | 19:08:33.90 +52:07:38.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1927AnHar.100...33C HD 234812 J-Ks=0.326+/-0.043 (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 2134205739425084288,2461058.9080,10.34,0.05,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 2134205739425084288 20260118.4080 10.34CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-11-Q1b1x1_2026-01-09_04-04-32_20.00sec_-15.00C_LIGHT_0081.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20.00sec_-15.00C_LIGHT_0458.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:08:33.88 +52:07:38.0 ;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_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4080 2461058.9080 13.21 19:08:53.99 +52:11:38.5
82.77785 18.58687 galactic Cyg Second-epoch detections are separated by 3.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J287.2227+52.1901 | 19:08:53.99 +52:11:38.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J287.2227+52.1901,2461058.9080,13.21,0.05,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
ATO J287.2227+52.1901 20260118.4080 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-11-Q1b1x1_2026-01-09_04-04-32_20.00sec_-15.00C_LIGHT_0081.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20.00sec_-15.00C_LIGHT_0458.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:08:53.99 +52:11:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4080 2461058.9080 13.23 19:09:58.98 +50:00:10.8
80.68983 17.64278 galactic Cyg Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:09:58.98 +50:00:10.8 (user input) | T | P | (position from user input) SpType: G5V 2016AJ....151...13G LAMOST J190959.17+500009.2 J-Ks=0.398+/-0.034 (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
target,2461058.9080,13.23,0.05,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
target 20260118.4080 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-11-Q1b1x1_2026-01-09_04-04-32_20.00sec_-15.00C_LIGHT_0081.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20.00sec_-15.00C_LIGHT_0458.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:09:58.98 +50:00:10.8 ;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_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4080 2461058.9080 13.30 18:58:54.40 +49:41:54.7
79.72961 19.20812 galactic Dra Second-epoch detections are separated by 2.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:58:54.40 +49:41:54.7 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.031 (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,2461058.9080,13.30,0.05,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 20260118.4080 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-11-Q1b1x1_2026-01-09_04-04-32_20.00sec_-15.00C_LIGHT_0081.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20.00sec_-15.00C_LIGHT_0458.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:58:54.40 +49:41:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4080 2461058.9080 13.76 18:53:34.53 +50:17:00.7
80.01971 20.20902 galactic Dra Second-epoch detections are separated by 3.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J283.3835+50.2842 | 18:53:34.53 +50:17:00.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.779+/-0.024 (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
ATO J283.3835+50.2842,2461058.9080,13.76,0.05,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
ATO J283.3835+50.2842 20260118.4080 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Dra-11-Q1b1x1_2026-01-09_04-04-32_20.00sec_-15.00C_LIGHT_0081.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Dra-11-Q1b1x1_060411_TTUQ1b1x1_8031_BrZpGz95/fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20.00sec_-15.00C_LIGHT_0458.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:53:34.53 +50:17:00.7 ;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_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-47-39_20_00sec_-15_00C_LIGHT_0458_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-11-Q1b1x1_2026-01-09_04-04-32_20_00sec_-15_00C_LIGHT_0081_fits__*pix.png resample_wcs_fd_Dra-11-Q1b1x1_2026-01-18_03-46-58_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4916 2461058.9916 14.05 16:41:24.80 +36:29:43.6
59.04621 40.97156 galactic Her Second-epoch detections are separated by 0.6" 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 | V1545 Her | 16:41:23.53 +36:30:17.2 (Gaia DR3) | SR: (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: K2Ib 1947ApJ...105..204P NGC 6205 70
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4916* 16 41 24.80 +36 29 43.6 14.1 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
V1545 Her,2461058.9916,14.05,0.05,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
V1545 Her 20260118.4916 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_062007_TTUQ1b1x1_13466_npF9VqLl/fd_CrB-01-Q1b1x1_2026-01-18_05-47-18_20.00sec_-15.00C_LIGHT_0547.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_CrB-01-Q1b1x1_062007_TTUQ1b1x1_13466_npF9VqLl/fd_CrB-01-Q1b1x1_2026-01-18_05-48-12_20.00sec_-14.90C_LIGHT_0548.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:41:24.80 +36:29:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_05-48-12_20_00sec_-14_90C_LIGHT_0548_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_05-47-18_20_00sec_-15_00C_LIGHT_0547_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_05-48-12_20_00sec_-14_90C_LIGHT_0548_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-01-18_05-47-18_20_00sec_-15_00C_LIGHT_0547_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 9.76 18:34:51.45 +26:13:27.2
55.05363 15.02270 galactic Lyr Second-epoch detections are separated by 1.7" and 9.8 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 4537247023944865152 | 18:34:51.95 +26:13:22.7 (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 4537247023944865152,2461058.9524,9.76,0.05,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 4537247023944865152 20260118.4524 9.76CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:34:51.45 +26:13:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 9.94 18:33:43.01 +26:02:40.8
54.77828 15.18736 galactic Her Second-epoch detections are separated by 2.8" and 9.5 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 4537237605078070272 | 18:33:42.62 +26:02:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4524* 18 33 43.01 +26 02 40.8 9.9 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 4537237605078070272,2461058.9524,9.94,0.05,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 4537237605078070272 20260118.4524 9.94CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:33:43.01 +26:02:40.8 ;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_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 10.03 18:35:29.54 +24:53:35.1
53.84943 14.36269 galactic Her Second-epoch detections are separated by 5.1" and 9.5 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 J278.8826+24.8979 | 18:35:31.01 +24:53:20.6 (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 01 18.4524* 18 35 29.54 +24 53 35.1 10.0 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
ATO J278.8826+24.8979,2461058.9524,10.03,0.05,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
ATO J278.8826+24.8979 20260118.4524 10.03CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:35:29.54 +24:53:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 10.44 18:33:17.43 +25:51:51.2
54.56731 15.20450 galactic Her Second-epoch detections are separated by 0.5" and 9.7 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 4537139890280705280 | 18:33:17.05 +25:51:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4524* 18 33 17.43 +25 51 51.2 10.4 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 4537139890280705280,2461058.9524,10.44,0.05,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 4537139890280705280 20260118.4524 10.44CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:33:17.43 +25:51:51.2 ;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_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 10.76 18:34:38.27 +25:46:09.4
54.60083 14.88842 galactic Her Second-epoch detections are separated by 1.3" and 9.6 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 J278.6671+25.7676 | 18:34:37.87 +25:46:12.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4524* 18 34 38.27 +25 46 09.4 10.8 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
ATO J278.6671+25.7676,2461058.9524,10.76,0.05,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
ATO J278.6671+25.7676 20260118.4524 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:34:38.27 +25:46:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 10.80 18:33:55.50 +26:05:24.2
54.84057 15.16223 galactic Her Second-epoch detections are separated by 1.1" and 9.7 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 4537239258643730176 | 18:33:55.04 +26:05:28.7 (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 01 18.4524* 18 33 55.50 +26 05 24.2 10.8 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 4537239258643730176,2461058.9524,10.80,0.05,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
Gaia DR3 4537239258643730176 20260118.4524 10.80CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:33:55.50 +26:05:24.2 ;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_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 10.86 18:35:11.74 +26:15:38.9
55.11939 14.96744 galactic Lyr Second-epoch detections are separated by 1.6" and 9.8 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 4537059862148040448 | 18:35:12.17 +26:15:34.3 (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 4537059862148040448,2461058.9524,10.86,0.05,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
Gaia DR3 4537059862148040448 20260118.4524 10.86CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:35:11.74 +26:15:38.9 ;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_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 10.99 18:35:00.90 +26:23:34.7
55.22864 15.05672 galactic Lyr Second-epoch detections are separated by 1.3" and 9.7 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 4537273068626624000 | 18:35:01.36 +26:23:31.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4537273068626624000,2461058.9524,10.99,0.05,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 4537273068626624000 20260118.4524 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:35:00.90 +26:23:34.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 11.19 18:33:16.14 +25:41:20.4
54.39845 15.13996 galactic Her Second-epoch detections are separated by 1.5" and 9.7 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 4536944177213231744 | 18:33:15.74 +25:41:24.0 (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 01 18.4524* 18 33 16.14 +25 41 20.4 11.2 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 4536944177213231744,2461058.9524,11.19,0.05,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 4536944177213231744 20260118.4524 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:33:16.14 +25:41:20.4 ;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_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 11.29 18:32:33.35 +24:54:03.4
53.58282 14.97666 galactic Her Second-epoch detections are separated by 1.8" and 9.7 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 4536460701333541504 | 18:32:32.97 +24:54:07.7 (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 01 18.4524* 18 32 33.35 +24 54 03.4 11.3 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 4536460701333541504,2461058.9524,11.29,0.05,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 4536460701333541504 20260118.4524 11.29CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:32:33.35 +24:54:03.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4524 2461058.9524 11.35 18:33:14.64 +25:28:41.2
54.19542 15.06196 galactic Her Second-epoch detections are separated by 0.7" and 9.7 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 4536925244997508736 | 18:33:14.20 +25:28:45.0 (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 01 18.4524* 18 33 14.64 +25 28 41.2 11.3 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 4536925244997508736,2461058.9524,11.35,0.05,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 4536925244997508736 20260118.4524 11.35CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-05-Q1b1x1_2026-01-09_05-16-42_20.00sec_-14.90C_LIGHT_0111.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20.00sec_-15.00C_LIGHT_0513.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-05-Q1b1x1_063215_TTUQ1b1x1_27721_BVGHSVtb/fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20.00sec_-14.90C_LIGHT_0514.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:33:14.64 +25:28:41.2 ;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_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-51-41_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-05-Q1b1x1_2026-01-09_05-16-42_20_00sec_-14_90C_LIGHT_0111_fits__*pix.png resample_wcs_fd_Her-05-Q1b1x1_2026-01-18_04-50-56_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4479 2461058.9479 9.54 18:01:15.63 +16:49:58.1
42.82395 18.48539 galactic Her Second-epoch detections are separated by 1.9" 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 4502268088730893696 | 18:01:16.02 +16:49:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1952CoRut..32....1H BD+16 3339
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4479* 18 01 15.63 +16 49 58.1 9.5 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 4502268088730893696,2461058.9479,9.54,0.05,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 4502268088730893696 20260118.4479 9.54CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-07-Q1b1x1_2026-01-09_05-09-31_20.00sec_-14.90C_LIGHT_0107.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-07-Q1b1x1_064402_TTUQ1b1x1_25719_zwHyGCFg/fd_Her-07-Q1b1x1_2026-01-18_04-44-30_20.00sec_-14.90C_LIGHT_0511.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-07-Q1b1x1_064402_TTUQ1b1x1_25719_zwHyGCFg/fd_Her-07-Q1b1x1_2026-01-18_04-45-13_20.00sec_-15.00C_LIGHT_0512.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:01:15.63 +16:49:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-07-Q1b1x1_2026-01-09_05-09-31_20_00sec_-14_90C_LIGHT_0107_fits__*pix.png resample_wcs_fd_Her-07-Q1b1x1_2026-01-18_04-45-13_20_00sec_-15_00C_LIGHT_0512_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-07-Q1b1x1_2026-01-09_05-09-31_20_00sec_-14_90C_LIGHT_0107_fits__*pix.png resample_wcs_fd_Her-07-Q1b1x1_2026-01-18_04-44-30_20_00sec_-14_90C_LIGHT_0511_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-07-Q1b1x1_2026-01-09_05-09-31_20_00sec_-14_90C_LIGHT_0107_fits__*pix.png resample_wcs_fd_Her-07-Q1b1x1_2026-01-18_04-45-13_20_00sec_-15_00C_LIGHT_0512_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-07-Q1b1x1_2026-01-09_05-09-31_20_00sec_-14_90C_LIGHT_0107_fits__*pix.png resample_wcs_fd_Her-07-Q1b1x1_2026-01-18_04-44-30_20_00sec_-14_90C_LIGHT_0511_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.5037 2461059.0037 9.21 17:04:57.59 +24:08:15.6
45.20619 33.39245 galactic Her Second-epoch detections are separated by 0.3" and 9.6 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 4571642668235608192 | 17:04:57.58 +24:08:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.030 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.5037* 17 04 57.59 +24 08 15.6 9.2 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 4571642668235608192,2461059.0037,9.21,0.05,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 4571642668235608192 20260118.5037 9.21CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-14-26_20.00sec_-15.00C_LIGHT_0085.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Her-06-Q1b1x1_2026-01-09_04-15-04_20.00sec_-15.00C_LIGHT_0086.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_064202_TTUQ1b1x1_27563_nZQszYuQ/fd_Her-06-Q1b1x1_2026-01-18_06-04-39_20.00sec_-15.00C_LIGHT_0011.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-06-Q1b1x1_064202_TTUQ1b1x1_27563_nZQszYuQ/fd_Her-06-Q1b1x1_2026-01-18_06-05-37_20.00sec_-14.90C_LIGHT_0012.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:04:57.59 +24:08:15.6 ;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_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_06-05-37_20_00sec_-14_90C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_06-04-39_20_00sec_-15_00C_LIGHT_0011_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_06-05-37_20_00sec_-14_90C_LIGHT_0012_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-06-Q1b1x1_2026-01-09_04-14-26_20_00sec_-15_00C_LIGHT_0085_fits__*pix.png resample_wcs_fd_Her-06-Q1b1x1_2026-01-18_06-04-39_20_00sec_-15_00C_LIGHT_0011_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3694* 09 51 06.00 +09 00 33.8 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
target,2461058.8694,14.45,0.05,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
target 20260118.3694 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Leo-04-Q1b1x1_040815_TTUQ1b1x1_2493_eq2V2p6i/fd_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Leo-04-Q1b1x1_040815_TTUQ1b1x1_2493_eq2V2p6i/fd_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:51:06.00 +09:00:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q1b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q1b1x1_2026-01-18_02-52-09_20_00sec_-14_90C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q1b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q1b1x1_2026-01-18_02-51-28_20_00sec_-15_00C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q1b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q1b1x1_2026-01-18_02-52-09_20_00sec_-14_90C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q1b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q1b1x1_2026-01-18_02-51-28_20_00sec_-15_00C_LIGHT_0400_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3694 2461058.8694 13.01 09:14:46.50 +11:13:06.0
219.29687 36.85503 galactic Cnc Second-epoch detections are separated by 0.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:14:46.50 +11:13:06.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.390+/-0.035 (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
target,2461058.8694,13.01,0.05,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
target 20260118.3694 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Leo-04-Q1b1x1_040815_TTUQ1b1x1_2493_eq2V2p6i/fd_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Leo-04-Q1b1x1_040815_TTUQ1b1x1_2493_eq2V2p6i/fd_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:14:46.50 +11:13:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q1b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q1b1x1_2026-01-18_02-52-09_20_00sec_-14_90C_LIGHT_0401_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q1b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q1b1x1_2026-01-18_02-51-28_20_00sec_-15_00C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q1b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q1b1x1_2026-01-18_02-52-09_20_00sec_-14_90C_LIGHT_0401_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q1b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q1b1x1_2026-01-18_02-51-28_20_00sec_-15_00C_LIGHT_0400_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.9996,14.28,0.05,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
target 20260118.4996 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Boo-08-Q1b1x1_2026-01-09_03-39-22_20.00sec_-15.00C_LIGHT_0068.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-08-Q1b1x1_063815_TTUQ1b1x1_14788_SZhu1zsj/fd_Boo-08-Q1b1x1_2026-01-18_05-58-53_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Boo-08-Q1b1x1_063815_TTUQ1b1x1_14788_SZhu1zsj/fd_Boo-08-Q1b1x1_2026-01-18_05-59-40_20.00sec_-15.00C_LIGHT_0006.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:57:21.14 +19:40:21.0 ;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_Boo-08-Q1b1x1_2026-01-09_03-39-22_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Boo-08-Q1b1x1_2026-01-18_05-59-40_20_00sec_-15_00C_LIGHT_0006_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-08-Q1b1x1_2026-01-09_03-39-22_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Boo-08-Q1b1x1_2026-01-18_05-58-53_20_00sec_-15_00C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-08-Q1b1x1_2026-01-09_03-39-22_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Boo-08-Q1b1x1_2026-01-18_05-59-40_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-08-Q1b1x1_2026-01-09_03-39-22_20_00sec_-15_00C_LIGHT_0068_fits__*pix.png resample_wcs_fd_Boo-08-Q1b1x1_2026-01-18_05-58-53_20_00sec_-15_00C_LIGHT_0005_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3931 2461058.8931 10.08 17:12:52.71 +42:19:45.6
67.25400 35.54668 galactic Her Second-epoch detections are separated by 0.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1354166805762941184 | 17:12:53.62 +42:19:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M1V 1926ApJ....64..225A BD+42 2810
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3931* 17 12 52.71 +42 19 45.6 10.1 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 1354166805762941184,2461058.8931,10.08,0.05,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 1354166805762941184 20260118.3931 10.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-01-Q1b1x1_2026-01-09_03-21-59_20.00sec_-15.00C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20.00sec_-15.00C_LIGHT_0435.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:12:52.71 +42:19:45.6 ;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_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3931 2461058.8931 11.16 17:19:53.37 +41:42:28.6
66.69298 34.17928 galactic Her Second-epoch detections are separated by 0.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1348028919540189056 | 17:19:53.12 +41:42:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M1/3 1923LicOB..11..127L LHS 3281
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.3931* 17 19 53.37 +41 42 28.6 11.2 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 1348028919540189056,2461058.8931,11.16,0.05,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 1348028919540189056 20260118.3931 11.16CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-01-Q1b1x1_2026-01-09_03-21-59_20.00sec_-15.00C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20.00sec_-15.00C_LIGHT_0435.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:19:53.37 +41:42:28.6 ;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_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3931 2461058.8931 13.07 17:17:20.00 +43:07:40.0
68.33360 34.81990 galactic Her Second-epoch detections are separated by 5.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J259.3332+43.1287 | 17:17:20.00 +43:07:40.0 (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 01 18.3931* 17 17 20.00 +43 07 40.0 13.1 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
ATO J259.3332+43.1287,2461058.8931,13.07,0.05,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
ATO J259.3332+43.1287 20260118.3931 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-01-Q1b1x1_2026-01-09_03-21-59_20.00sec_-15.00C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20.00sec_-15.00C_LIGHT_0435.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:17:20.00 +43:07:40.0 ;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_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3931 2461058.8931 13.02 17:17:20.19 +43:08:24.8
68.34875 34.82069 galactic Her Second-epoch detections are separated by 3.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 | 17:17:20.19 +43:08:24.8 (user input) | 1360404781907157632 (VSX @ VizieR) | E (VSX @ VizieR) | (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 01 18.3931* 17 17 20.19 +43 08 24.8 13.0 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 DR3,2461058.8931,13.02,0.05,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
Gaia DR3 20260118.3931 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-01-Q1b1x1_2026-01-09_03-21-59_20.00sec_-15.00C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20.00sec_-15.00C_LIGHT_0435.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:17:20.19 +43:08:24.8 ;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_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3931 2461058.8931 13.93 17:20:41.92 +43:52:42.2
69.32081 34.29567 galactic Her Second-epoch detections are separated by 4.4" 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 J260.1763+43.8765 | 17:20:41.92 +43:52:42.2 (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 01 18.3931* 17 20 41.92 +43 52 42.2 13.9 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
ATO J260.1763+43.8765,2461058.8931,13.93,0.05,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
ATO J260.1763+43.8765 20260118.3931 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-01-Q1b1x1_2026-01-09_03-21-59_20.00sec_-15.00C_LIGHT_0050.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20.00sec_-15.00C_LIGHT_0435.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-01-Q1b1x1_060808_TTUQ1b1x1_6734_O3wnigXu/fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20.00sec_-15.00C_LIGHT_0436.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:20:41.92 +43:52:42.2 ;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_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-26-14_20_00sec_-15_00C_LIGHT_0436_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-01-Q1b1x1_2026-01-09_03-21-59_20_00sec_-15_00C_LIGHT_0050_fits__*pix.png resample_wcs_fd_Her-01-Q1b1x1_2026-01-18_03-25-29_20_00sec_-15_00C_LIGHT_0435_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.5131 2461059.0131 7.87 16:30:27.59 +04:10:06.0
19.28610 33.04984 galactic Her Second-epoch detections are separated by 0.7" 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 4433711099194059904 | 16:30:27.99 +04:10:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7V 1935ApJ....81..187A HD 148816
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.5131* 16 30 27.59 +04 10 06.0 7.9 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 4433711099194059904,2461059.0131,7.87,0.05,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 4433711099194059904 20260118.5131 7.87CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-11-Q1b1x1_2026-01-09_04-36-02_20.00sec_-14.90C_LIGHT_0097.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-11-Q1b1x1_070021_TTUQ1b1x1_26915_pKXSqjzd/fd_Her-11-Q1b1x1_2026-01-18_06-18-15_20.00sec_-14.90C_LIGHT_0025.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-11-Q1b1x1_070021_TTUQ1b1x1_26915_pKXSqjzd/fd_Her-11-Q1b1x1_2026-01-18_06-19-11_20.00sec_-14.90C_LIGHT_0026.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:30:27.59 +04:10:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-11-Q1b1x1_2026-01-09_04-36-02_20_00sec_-14_90C_LIGHT_0097_fits__*pix.png resample_wcs_fd_Her-11-Q1b1x1_2026-01-18_06-19-11_20_00sec_-14_90C_LIGHT_0026_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-11-Q1b1x1_2026-01-09_04-36-02_20_00sec_-14_90C_LIGHT_0097_fits__*pix.png resample_wcs_fd_Her-11-Q1b1x1_2026-01-18_06-18-15_20_00sec_-14_90C_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_Her-11-Q1b1x1_2026-01-09_04-36-02_20_00sec_-14_90C_LIGHT_0097_fits__*pix.png resample_wcs_fd_Her-11-Q1b1x1_2026-01-18_06-19-11_20_00sec_-14_90C_LIGHT_0026_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-11-Q1b1x1_2026-01-09_04-36-02_20_00sec_-14_90C_LIGHT_0097_fits__*pix.png resample_wcs_fd_Her-11-Q1b1x1_2026-01-18_06-18-15_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.5131 2461059.0131 9.66 16:44:54.44 +06:48:17.4
24.05692 31.16560 galactic Her Second-epoch detections are separated by 0.1" 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 | ATO J251.2311+06.8106 | 16:44:54.46 +06:48:17.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.793+/-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!
TCP 2026 01 18.5131* 16 44 54.44 +06 48 17.4 9.7 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
ATO J251.2311+06.8106,2461059.0131,9.66,0.05,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
ATO J251.2311+06.8106 20260118.5131 9.66CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-11-Q1b1x1_2026-01-09_04-36-02_20.00sec_-14.90C_LIGHT_0097.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Her-11-Q1b1x1_2026-01-09_04-36-40_20.00sec_-15.00C_LIGHT_0098.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-11-Q1b1x1_070021_TTUQ1b1x1_26915_pKXSqjzd/fd_Her-11-Q1b1x1_2026-01-18_06-18-15_20.00sec_-14.90C_LIGHT_0025.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-11-Q1b1x1_070021_TTUQ1b1x1_26915_pKXSqjzd/fd_Her-11-Q1b1x1_2026-01-18_06-19-11_20.00sec_-14.90C_LIGHT_0026.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:44:54.44 +06:48:17.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-11-Q1b1x1_2026-01-09_04-36-02_20_00sec_-14_90C_LIGHT_0097_fits__*pix.png resample_wcs_fd_Her-11-Q1b1x1_2026-01-18_06-19-11_20_00sec_-14_90C_LIGHT_0026_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-11-Q1b1x1_2026-01-09_04-36-02_20_00sec_-14_90C_LIGHT_0097_fits__*pix.png resample_wcs_fd_Her-11-Q1b1x1_2026-01-18_06-18-15_20_00sec_-14_90C_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_Her-11-Q1b1x1_2026-01-09_04-36-02_20_00sec_-14_90C_LIGHT_0097_fits__*pix.png resample_wcs_fd_Her-11-Q1b1x1_2026-01-18_06-19-11_20_00sec_-14_90C_LIGHT_0026_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-11-Q1b1x1_2026-01-09_04-36-02_20_00sec_-14_90C_LIGHT_0097_fits__*pix.png resample_wcs_fd_Her-11-Q1b1x1_2026-01-18_06-18-15_20_00sec_-14_90C_LIGHT_0025_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4363 2461058.9363 12.33 17:25:11.68 +10:49:40.8
33.09556 24.01019 galactic Oph Second-epoch detections are separated by 1.6" and 10.6 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 4492109288482343296 | 17:25:12.05 +10:49:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4492109288482343296,2461058.9363,12.33,0.05,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
Gaia DR3 4492109288482343296 20260118.4363 12.33CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:11.68 +10:49:40.8 ;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_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4363 2461058.9363 12.98 17:25:18.08 +08:51:50.6
31.17239 23.14357 galactic Oph Second-epoch detections are separated by 0.7" and 11.4 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 4490585395427304576 | 17:25:18.41 +08:51:47.0 (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 4490585395427304576,2461058.9363,12.98,0.05,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 4490585395427304576 20260118.4363 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:18.08 +08:51:50.6 ;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_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4363 2461058.9363 13.16 17:25:31.40 +10:24:47.1
32.72214 23.76099 galactic Oph Second-epoch detections are separated by 2.2" and 11.1 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 4491901343345516032 | 17:25:31.76 +10:24:44.4 (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 4491901343345516032,2461058.9363,13.16,0.05,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
Gaia DR3 4491901343345516032 20260118.4363 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:31.40 +10:24:47.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4363 2461058.9363 13.16 17:25:18.23 +10:42:26.9
32.98849 23.93486 galactic Oph Second-epoch detections are separated by 1.2" and 10.7 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 4492104306320423040 | 17:25:18.60 +10:42:23.8 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4492104306320423040,2461058.9363,13.16,0.05,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
Gaia DR3 4492104306320423040 20260118.4363 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:18.23 +10:42:26.9 ;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_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4363 2461058.9363 13.15 17:14:35.37 +09:26:40.7
30.48604 25.77733 galactic Oph Second-epoch detections are separated by 4.6" and 10.8 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 | 17:14:35.37 +09:26:40.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.9363,13.15,0.05,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
target 20260118.4363 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:14:35.37 +09:26:40.7 ;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_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4363 2461058.9363 13.22 17:25:27.76 +08:55:38.9
31.25334 23.13527 galactic Oph Second-epoch detections are separated by 0.9" and 11.4 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 4490591550118647424 | 17:25:28.15 +08:55:35.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4490591550118647424,2461058.9363,13.22,0.05,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
Gaia DR3 4490591550118647424 20260118.4363 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:27.76 +08:55:38.9 ;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_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4363 2461058.9363 13.30 17:25:06.04 +10:37:30.8
32.88383 23.94519 galactic Oph Second-epoch detections are separated by 1.3" and 10.5 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 J261.2766+10.6244 | 17:25:06.04 +10:37:30.8 (user input) | LPV (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 J261.2766+10.6244,2461058.9363,13.30,0.05,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 J261.2766+10.6244 20260118.4363 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:06.04 +10:37:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.9363,13.31,0.05,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
target 20260118.4363 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:19.77 +10:57:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4363* 17 15 52.39 +18 45 43.7 13.4 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
target,2461058.9363,13.43,0.05,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
target 20260118.4363 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:15:52.39 +18:45:43.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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,2461058.9363,13.72,0.05,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
target 20260118.4363 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:06.54 +10:36:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4363 2461058.9363 13.56 17:25:12.94 +10:42:30.8
32.97952 23.95494 galactic Oph Second-epoch detections are separated by 3.4" and 10.9 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 4492098632665407360 | 17:25:13.37 +10:42:27.9 (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 4492098632665407360,2461058.9363,13.56,0.05,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
Gaia DR3 4492098632665407360 20260118.4363 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-09-Q1b1x1_2026-01-09_04-51-29_20.00sec_-14.90C_LIGHT_0103.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20.00sec_-15.00C_LIGHT_0503.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-09-Q1b1x1_065207_TTUQ1b1x1_12616_gaUBsr2l/fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20.00sec_-15.00C_LIGHT_0504.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:12.94 +10:42:30.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-28-39_20_00sec_-15_00C_LIGHT_0504_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-09-Q1b1x1_2026-01-09_04-51-29_20_00sec_-14_90C_LIGHT_0103_fits__*pix.png resample_wcs_fd_Her-09-Q1b1x1_2026-01-18_04-27-26_20_00sec_-15_00C_LIGHT_0503_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4146 2461058.9146 13.41 17:16:57.27 +43:05:23.6
68.27850 34.88449 galactic Her Second-epoch detections are separated by 1.5" and 4.0 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 1360404983765400960 | 17:16:56.78 +43:05:36.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4146* 17 16 57.27 +43 05 23.6 13.4 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 1360404983765400960,2461058.9146,13.41,0.05,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
Gaia DR3 1360404983765400960 20260118.4146 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-03-Q1b1x1_2026-01-09_04-18-34_20.00sec_-14.90C_LIGHT_0089.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20.00sec_-14.90C_LIGHT_0467.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20.00sec_-15.00C_LIGHT_0468.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:16:57.27 +43:05:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4146 2461058.9146 12.04 18:05:23.76 +32:52:50.3
59.23433 23.37166 galactic Her Second-epoch detections are separated by 3.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J271.3433+32.8756 | 18:05:24.26 +32:52:46.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4146* 18 05 23.76 +32 52 50.3 12.0 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
ATO J271.3433+32.8756,2461058.9146,12.04,0.05,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 J271.3433+32.8756 20260118.4146 12.04CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-03-Q1b1x1_2026-01-09_04-18-34_20.00sec_-14.90C_LIGHT_0089.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20.00sec_-14.90C_LIGHT_0467.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20.00sec_-15.00C_LIGHT_0468.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:05:23.76 +32:52:50.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4146 2461058.9146 12.34 18:05:42.35 +32:57:48.4
59.34213 23.33574 galactic Her Second-epoch detections are separated by 3.3" 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 4603667559302129792 | 18:05:42.82 +32:57:44.8 (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 01 18.4146* 18 05 42.35 +32 57 48.4 12.3 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 4603667559302129792,2461058.9146,12.34,0.05,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 4603667559302129792 20260118.4146 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-03-Q1b1x1_2026-01-09_04-18-34_20.00sec_-14.90C_LIGHT_0089.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20.00sec_-14.90C_LIGHT_0467.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20.00sec_-15.00C_LIGHT_0468.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:05:42.35 +32:57:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4146 2461058.9146 12.63 18:01:15.23 +35:19:54.3
61.51554 24.92421 galactic Her Second-epoch detections are separated by 1.6" and 4.0 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 4604907391803729664 | 18:01:15.11 +35:20:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4146* 18 01 15.23 +35 19 54.3 12.6 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 4604907391803729664,2461058.9146,12.63,0.05,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 4604907391803729664 20260118.4146 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-03-Q1b1x1_2026-01-09_04-18-34_20.00sec_-14.90C_LIGHT_0089.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20.00sec_-14.90C_LIGHT_0467.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20.00sec_-15.00C_LIGHT_0468.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:01:15.23 +35:19:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4146 2461058.9146 13.57 16:55:22.02 +32:41:32.4
54.74561 37.56160 galactic Her Second-epoch detections are separated by 1.6" and 4.0 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 | 16:55:22.02 +32:41:32.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4146* 16 55 22.02 +32 41 32.4 13.6 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
target,2461058.9146,13.57,0.05,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 20260118.4146 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-03-Q1b1x1_2026-01-09_04-18-34_20.00sec_-14.90C_LIGHT_0089.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20.00sec_-14.90C_LIGHT_0467.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-03-Q1b1x1_062206_TTUQ1b1x1_27617_DUOAMZYo/fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20.00sec_-15.00C_LIGHT_0468.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:55:22.02 +32:41:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-57-10_20_00sec_-15_00C_LIGHT_0468_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q1b1x1_2026-01-09_04-18-34_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png resample_wcs_fd_Her-03-Q1b1x1_2026-01-18_03-56-32_20_00sec_-14_90C_LIGHT_0467_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.5192 2461059.0192 7.79 15:43:00.97 -10:56:08.0
356.30380 33.61915 galactic Lib Second-epoch detections are separated by 0.1" 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 | NSV 7210 | 15:43:01.89 -10:56:05.5 (Gaia DR3) | CST (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: F5 1921AnHar..96.....C HD 140283
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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
NSV 7210,2461059.0192,7.79,0.05,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
NSV 7210 20260118.5192 7.79CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lib-02-Q1b1x1_2026-01-09_04-30-36_20.00sec_-15.00C_LIGHT_0093.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-02-Q1b1x1_071829_TTUQ1b1x1_326_p8HdjvXH/fd_Lib-02-Q1b1x1_2026-01-18_06-27-06_20.00sec_-15.00C_LIGHT_0035.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lib-02-Q1b1x1_071829_TTUQ1b1x1_326_p8HdjvXH/fd_Lib-02-Q1b1x1_2026-01-18_06-28-00_20.00sec_-14.90C_LIGHT_0036.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:43:00.97 -10:56:08.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-02-Q1b1x1_2026-01-09_04-30-36_20_00sec_-15_00C_LIGHT_0093_fits__*pix.png resample_wcs_fd_Lib-02-Q1b1x1_2026-01-18_06-28-00_20_00sec_-14_90C_LIGHT_0036_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-02-Q1b1x1_2026-01-09_04-30-36_20_00sec_-15_00C_LIGHT_0093_fits__*pix.png resample_wcs_fd_Lib-02-Q1b1x1_2026-01-18_06-27-06_20_00sec_-15_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-02-Q1b1x1_2026-01-09_04-30-36_20_00sec_-15_00C_LIGHT_0093_fits__*pix.png resample_wcs_fd_Lib-02-Q1b1x1_2026-01-18_06-28-00_20_00sec_-14_90C_LIGHT_0036_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-02-Q1b1x1_2026-01-09_04-30-36_20_00sec_-15_00C_LIGHT_0093_fits__*pix.png resample_wcs_fd_Lib-02-Q1b1x1_2026-01-18_06-27-06_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 14.29 06:54:33.86 +21:41:38.5
193.75046 10.36014 galactic Gem Second-epoch detections are separated by 1.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.6313+21.6989 | 06:54:33.86 +21:41:38.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.6313+21.6989,2461058.7379,14.29,0.05,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
ATO J103.6313+21.6989 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:54:33.86 +21:41:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 12.59 07:56:45.88 +23:46:51.0
197.55285 24.38615 galactic Gem Second-epoch detections are separated by 0.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 681241873969141888 | 07:56:45.25 +23:46:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.655+/-0.029 (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 681241873969141888,2461058.7379,12.59,0.05,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
Gaia DR3 681241873969141888 20260118.2379 12.59CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:56:45.88 +23:46:51.0 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 12.23 07:50:52.64 +26:16:04.0
194.49100 23.98368 galactic Gem Second-epoch detections are separated by 0.3" 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 874097214210138368 | 07:50:52.64 +26:16:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.274+/-0.029 (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 874097214210138368,2461058.7379,12.23,0.05,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
Gaia DR3 874097214210138368 20260118.2379 12.23CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:52.64 +26:16:04.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 13.42 07:50:00.90 +23:50:31.8
196.89890 22.96196 galactic Gem Second-epoch detections are separated by 0.6" 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 | target | 07:50:00.90 +23:50:31.8 (user input) | T | P | (position from user input) J-Ks=0.676+/-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,2461058.7379,13.42,0.05,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
target 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:00.90 +23:50:31.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 12.42 06:52:47.73 +17:45:33.8
197.16478 8.28545 galactic Gem Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3364488027466925568 | 06:52:47.71 +17:45:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.266+/-0.030 (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 3364488027466925568,2461058.7379,12.42,0.05,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 3364488027466925568 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:52:47.73 +17:45:33.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 12.94 06:52:57.18 +16:45:59.6
198.08284 7.88425 galactic Gem Second-epoch detections are separated by 2.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:52:57.18 +16:45:59.6 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.7379,12.94,0.05,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
target 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:52:57.18 +16:45:59.6 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 11.60 07:48:13.23 +26:50:31.9
193.68120 23.61765 galactic Gem Second-epoch detections are separated by 0.6" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 874892882670502272 | 07:48:13.20 +26:50:32.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.356+/-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 874892882670502272,2461058.7379,11.60,0.05,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
Gaia DR3 874892882670502272 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:48:13.23 +26:50:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 13.20 06:51:19.49 +16:46:34.2
197.90117 7.53846 galactic Gem Second-epoch detections are separated by 4.2" 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 | target | 06:51:19.49 +16:46:34.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.7379,13.20,0.05,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 20260118.2379 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:19.49 +16:46:34.2 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 11.93 07:53:40.89 +25:14:13.5
195.78774 24.22854 galactic Gem Second-epoch detections are separated by 0.1" 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 | ATO J118.4162+25.2388 | 07:53:40.88 +25:14:13.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.425+/-0.028 (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 J118.4162+25.2388,2461058.7379,11.93,0.05,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
ATO J118.4162+25.2388 20260118.2379 11.93CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:53:40.89 +25:14:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 13.22 06:51:08.02 +17:57:17.7
196.81229 8.01553 galactic Gem Second-epoch detections are separated by 0.4" 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 | target | 06:51:08.02 +17:57:17.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.651+/-0.027 (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,2461058.7379,13.22,0.05,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
target 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:08.02 +17:57:17.7 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 12.94 07:50:53.26 +26:30:03.7
194.25134 24.06427 galactic Gem Second-epoch detections are separated by 0.7" 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 | target | 07:50:53.26 +26:30:03.7 (user input) | T | P | (position from user input) SpType: A7IV (LAMOST DR5) J-Ks=0.185+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.7379,12.94,0.05,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
target 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:53.26 +26:30:03.7 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 13.31 07:46:27.08 +26:39:36.1
193.72242 23.18436 galactic Gem Second-epoch detections are separated by 0.5" 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 | target | 07:46:27.08 +26:39:36.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.546+/-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,2461058.7379,13.31,0.05,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
target 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:27.08 +26:39:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 12.69 06:51:34.03 +16:44:23.0
197.95995 7.57449 galactic Gem Second-epoch detections are separated by 4.5" 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 | Gaia DR3 3358118414869900544 | 06:51:34.03 +16:44:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.727+/-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 3358118414869900544,2461058.7379,12.69,0.05,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
Gaia DR3 3358118414869900544 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:34.03 +16:44:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.2379 2461058.7379 12.69 07:51:54.56 +25:55:16.7
194.93372 24.08484 galactic Gem Second-epoch detections are separated by 0.1" 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 | Large-amplitude variable Gaia DR2 874027154703904768 | 07:51:54.56 +25:55:16.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F5 (LAMOST DR5) J-Ks=0.258+/-0.028 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 874027154703904768,2461058.7379,12.69,0.05,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
Large-amplitude variable Gaia DR2 874027154703904768 20260118.2379 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2025-12-23_03-02-35_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20.00sec_-14.90C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Gem-04-Q1b1x1_033657_TTUQ1b1x1_3917_jHpfRmeZ/fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20.00sec_-15.00C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:54.56 +25:55:16.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-42-48_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-17_23-41-58_20_00sec_-14_90C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 9.95 17:35:21.77 +25:26:33.0
49.13997 27.24476 galactic Her Second-epoch detections are separated by 0.6" 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 | ATO J263.8333+25.4326 | 17:35:22.31 +25:26:28.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 35 21.77 +25 26 33.0 9.9 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
ATO J263.8333+25.4326,2461058.9122,9.95,0.05,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
ATO J263.8333+25.4326 20260118.4122 9.95CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:35:21.77 +25:26:33.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 10.71 17:27:43.43 +26:08:19.3
49.27366 29.09610 galactic Her Second-epoch detections are separated by 5.8" 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 4570834905146140416 | 17:27:43.42 +26:08:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=4.142+/- (unrealisitic color!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 27 43.43 +26 08 19.3 10.7 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 4570834905146140416,2461058.9122,10.71,0.05,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
Gaia DR3 4570834905146140416 20260118.4122 10.71CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:27:43.43 +26:08:19.3 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 11.04 17:29:51.59 +26:12:53.8
49.52567 28.66391 galactic Her Second-epoch detections are separated by 1.8" 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 4570846793615521152 | 17:29:51.87 +26:12:48.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 29 51.59 +26 12 53.8 11.0 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 4570846793615521152,2461058.9122,11.04,0.05,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 4570846793615521152 20260118.4122 11.04CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:29:51.59 +26:12:53.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 11.80 17:35:21.50 +24:48:26.7
48.46480 27.03898 galactic Her Second-epoch detections are separated by 4.1" 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 | Gaia DR3 4569719931636748160 | 17:35:21.97 +24:48:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 35 21.50 +24 48 26.7 11.8 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 4569719931636748160,2461058.9122,11.80,0.05,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
Gaia DR3 4569719931636748160 20260118.4122 11.80CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:35:21.50 +24:48:26.7 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 12.29 17:30:05.36 +26:22:18.6
49.71383 28.66356 galactic Her Second-epoch detections are separated by 1.2" 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 4594872290914486784 | 17:30:05.64 +26:22:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 30 05.36 +26 22 18.6 12.3 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 4594872290914486784,2461058.9122,12.29,0.05,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 4594872290914486784 20260118.4122 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:30:05.36 +26:22:18.6 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 12.60 17:29:51.52 +26:09:14.2
49.45949 28.64523 galactic Her Second-epoch detections are separated by 2.1" 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 4570845934622211456 | 17:29:51.79 +26:09:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 29 51.52 +26 09 14.2 12.6 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 4570845934622211456,2461058.9122,12.60,0.05,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 4570845934622211456 20260118.4122 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:29:51.52 +26:09:14.2 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 12.62 17:28:30.13 +25:48:12.6
48.97145 28.82584 galactic Her Second-epoch detections are separated by 1.3" 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 4570763776189886464 | 17:28:30.49 +25:48:08.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 28 30.13 +25 48 12.6 12.6 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 4570763776189886464,2461058.9122,12.62,0.05,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
Gaia DR3 4570763776189886464 20260118.4122 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:28:30.13 +25:48:12.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 13.05 17:29:15.17 +25:57:16.6
49.19531 28.71253 galactic Her Second-epoch detections are separated by 0.6" 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 | ATO J262.3141+25.9531 | 17:29:15.39 +25:57:11.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 29 15.17 +25 57 16.6 13.1 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
ATO J262.3141+25.9531,2461058.9122,13.05,0.05,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
ATO J262.3141+25.9531 20260118.4122 13.05CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:29:15.17 +25:57:16.6 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 13.30 17:27:03.77 +25:12:00.1
48.20065 28.94482 galactic Her Second-epoch detections are separated by 1.9" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 17:27:03.77 +25:12:00.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 27 03.77 +25 12 00.1 13.3 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
target,2461058.9122,13.30,0.05,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 20260118.4122 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:27:03.77 +25:12:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 29 04.27 +26 01 18.4 13.3 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
target,2461058.9122,13.28,0.05,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
target 20260118.4122 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:29:04.27 +26:01:18.4 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 30 09.58 +25 55 41.6 13.3 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
target,2461058.9122,13.34,0.05,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
target 20260118.4122 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:30:09.58 +25:55:41.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 25 42.42 +25 26 14.7 13.6 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
target,2461058.9122,13.58,0.05,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
target 20260118.4122 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:42.42 +25:26:14.7 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 13.38 17:13:19.77 +26:55:49.3
49.04529 32.40557 galactic Her Second-epoch detections are separated by 8.3" 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 J258.3367+26.9333 | 17:13:19.77 +26:55:49.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 13 19.77 +26 55 49.3 13.4 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
ATO J258.3367+26.9333,2461058.9122,13.38,0.05,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
ATO J258.3367+26.9333 20260118.4122 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:13:19.77 +26:55:49.3 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 13.69 17:30:11.31 +26:31:44.1
49.89195 28.69089 galactic Her Second-epoch detections are separated by 1.8" 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 J262.5369+26.5211 | 17:30:11.31 +26:31:44.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 30 11.31 +26 31 44.1 13.7 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
ATO J262.5369+26.5211,2461058.9122,13.69,0.05,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
ATO J262.5369+26.5211 20260118.4122 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:30:11.31 +26:31:44.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.4122 2461058.9122 13.71 17:27:23.97 +25:23:04.8
48.42828 28.93076 galactic Her Second-epoch detections are separated by 4.5" 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 | 17:27:23.97 +25:23:04.8 (user input) | T | P | (position from user input) SpType: G9 (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 01 18.4122* 17 27 23.97 +25 23 04.8 13.7 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
target,2461058.9122,13.71,0.05,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
target 20260118.4122 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:27:23.97 +25:23:04.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 18.4122* 17 25 41.48 +25 24 40.1 13.7 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
target,2461058.9122,13.68,0.05,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
target 20260118.4122 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Her-04-Q1b1x1_2026-01-09_04-16-04_20.00sec_-15.00C_LIGHT_0087.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20.00sec_-14.90C_LIGHT_0463.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Her-04-Q1b1x1_063013_TTUQ1b1x1_15699_phWw9KBq/fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20.00sec_-14.90C_LIGHT_0464.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:41.48 +25:24:40.1 ;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_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-53-48_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-04-Q1b1x1_2026-01-09_04-16-04_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png resample_wcs_fd_Her-04-Q1b1x1_2026-01-18_03-52-54_20_00sec_-14_90C_LIGHT_0463_fits__*pix.png animation_v2.gif