Mean magnitude and position on the discovery images:
2026 01 21.2326 2461061.7326 14.19 09:03:39.82 +03:22:08.1
226.11573 30.75807 galactic Hya 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 578306596103857152 | 09:03:39.44 +03:21:25.3 (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 578306596103857152,2461061.7326,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 578306596103857152 20260121.2326 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Hya-01-Q1b1x1_235717_TTUQ1b1x1_26225_gnlw5i0w/fd_Hya-01-Q1b1x1_2026-01-20_23-34-28_20.00sec_-14.90C_LIGHT_0252.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Hya-01-Q1b1x1_235717_TTUQ1b1x1_26225_gnlw5i0w/fd_Hya-01-Q1b1x1_2026-01-20_23-35-08_20.00sec_-15.00C_LIGHT_0253.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:39.82 +03:22:08.1 ;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-01-Q1b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q1b1x1_2026-01-20_23-35-08_20_00sec_-15_00C_LIGHT_0253_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_2026-01-20_23-34-28_20_00sec_-14_90C_LIGHT_0252_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_2026-01-20_23-35-08_20_00sec_-15_00C_LIGHT_0253_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_2026-01-20_23-34-28_20_00sec_-14_90C_LIGHT_0252_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0967 2461061.5967 14.07 06:31:19.12 +18:17:55.8
194.38091 3.96135 galactic Gem Second-epoch detections are separated by 1.0" 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 | EPIC 202091663 | 06:31:16.96 +18:17:43.7 (Gaia DR3) | VAR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.370+/-0.066 (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
EPIC 202091663,2461061.5967,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 202091663 20260121.0967 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2025-12-23_02-10-23_20.00sec_-14.90C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20.00sec_-14.90C_LIGHT_0056.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20.00sec_-15.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:19.12 +18:17:55.8 ;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_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0967 2461061.5967 14.44 05:59:14.19 +17:11:60.0
191.70097 -3.27568 galactic Ori Second-epoch detections are separated by 2.3" 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 | ATO J089.8156+17.1852 | 05:59:13.57 +17:11:30.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.0967* 05 59 14.19 +17 11 60.0 14.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.8156+17.1852,2461061.5967,14.44,0.05,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 J089.8156+17.1852 20260121.0967 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/Gem-03-Q1b1x1_2025-12-23_02-10-23_20.00sec_-14.90C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20.00sec_-14.90C_LIGHT_0056.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20.00sec_-15.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:14.19 +17:11:60.0 ;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_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0967 2461061.5967 14.36 06:02:33.43 +23:28:55.5
186.62568 0.51053 galactic Gem Second-epoch detections are separated by 3.6" 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 3424676148667976832 | 06:02:31.31 +23:29:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1967AJ.....72.1199M [M67b] +23 348
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3424676148667976832,2461061.5967,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3424676148667976832 20260121.0967 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2025-12-23_02-10-23_20.00sec_-14.90C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20.00sec_-14.90C_LIGHT_0056.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20.00sec_-15.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:33.43 +23:28:55.5 ;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_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0967 2461061.5967 14.46 06:41:04.16 +22:47:21.0
191.38062 8.01965 galactic Gem Second-epoch detections are separated by 2.8" 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 | ATO J100.2684+22.7867 | 06:41:04.16 +22:47:21.0 (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 J100.2684+22.7867,2461061.5967,14.46,0.05,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 J100.2684+22.7867 20260121.0967 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/Gem-03-Q1b1x1_2025-12-23_02-10-23_20.00sec_-14.90C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20.00sec_-14.90C_LIGHT_0056.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20.00sec_-15.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:04.16 +22:47:21.0 ;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_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0967 2461061.5967 13.74 06:28:02.60 +17:34:42.7
194.66192 2.93810 galactic Gem Second-epoch detections are separated by 4.8" 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 | ATO J097.0101+17.5763 | 06:28:02.60 +17:34:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.0101+17.5763,2461061.5967,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.0101+17.5763 20260121.0967 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2025-12-23_02-10-23_20.00sec_-14.90C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2025-12-23_02-11-12_20.00sec_-14.90C_LIGHT_0417.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20.00sec_-14.90C_LIGHT_0056.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-03-Q1b1x1_212140_TTUQ1b1x1_11835_OHq3Gjmi/fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20.00sec_-15.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:02.60 +17:34:42.7 ;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_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-19-29_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-20_20-18-41_20_00sec_-14_90C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 9.19 07:39:05.81 -22:50:12.1
238.53812 -0.43715 galactic Pup Second-epoch detections are separated by 1.7" 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 | 07:39:06.61 -22:50:21.0 (Gaia DR3) | 5615842126631520128 (VSX @ VizieR) | VAR (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE SpType: K3/4 1988MSS...C04....0H HD 61592
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3,2461061.5883,9.19,0.05,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 20260121.0883 9.19CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:05.81 -22:50:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 9.39 07:33:13.09 -21:56:18.2
237.09127 -1.18584 galactic Pup Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J113.3054-21.9250 | 07:33:13.20 -21:56:15.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5/7V 1988MSS...C04....0H HD 60343
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J113.3054-21.9250,2461061.5883,9.39,0.05,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 J113.3054-21.9250 20260121.0883 9.39CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:13.09 -21:56:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 10.03 07:39:04.90 -23:04:35.5
238.74528 -0.55808 galactic Pup Second-epoch detections are separated by 1.0" 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 | ATO J114.7786-23.0689 | 07:39:05.79 -23:04:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J114.7786-23.0689,2461061.5883,10.03,0.05,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 J114.7786-23.0689 20260121.0883 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:04.90 -23:04:35.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 10.37 07:40:19.15 -22:49:11.3
238.66213 -0.18371 galactic Pup Second-epoch detections are separated by 0.7" 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 5615921531991236608 | 07:40:20.18 -22:49:22.1 (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 5615921531991236608,2461061.5883,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5615921531991236608 20260121.0883 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:40:19.15 -22:49:11.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 10.52 07:27:00.89 -21:09:54.1
235.72069 -2.08119 galactic CMa Second-epoch detections are separated by 0.5" 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 | ATO J111.7505-21.1572 | 07:27:01.12 -21:09:49.1 (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 J111.7505-21.1572,2461061.5883,10.52,0.05,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
ATO J111.7505-21.1572 20260121.0883 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:27:00.89 -21:09:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 10.79 07:24:03.77 -21:40:33.4
235.84589 -2.92818 galactic CMa Second-epoch detections are separated by 1.1" 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 | ATO J111.0113-21.6684 | 07:24:04.14 -21:40:29.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J111.0113-21.6684,2461061.5883,10.79,0.05,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 J111.0113-21.6684 20260121.0883 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:24:03.77 -21:40:33.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 10.71 07:38:52.45 -22:56:46.8
238.60842 -0.53569 galactic Pup Second-epoch detections are separated by 0.4" 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 J114.7182-22.9415 | 07:38:53.27 -22:56:55.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5V 1970AJ.....75..324W LF 12 36
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J114.7182-22.9415,2461061.5883,10.71,0.05,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
ATO J114.7182-22.9415 20260121.0883 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:38:52.45 -22:56:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 11.18 07:36:28.73 -21:48:11.2
237.34043 -0.45885 galactic Pup Second-epoch detections are separated by 3.8" 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 | 07:36:28.88 -21:48:00.6 (Gaia DR3) | 5619235150797344896 (VSX @ VizieR) | DSCT|GDOR|SXPHE (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3,2461061.5883,11.18,0.05,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 20260121.0883 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:28.73 -21:48:11.2 ;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-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 11.31 07:37:51.98 -21:01:52.7
236.82503 0.20019 galactic Pup Second-epoch detections are separated by 2.4" 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 J114.4636-21.0248 | 07:37:52.14 -21:01:52.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.238+/-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 J114.4636-21.0248,2461061.5883,11.31,0.05,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 J114.4636-21.0248 20260121.0883 11.31CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:51.98 -21:01:52.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 11.29 07:39:23.95 -22:54:25.0
238.63354 -0.41106 galactic Pup Second-epoch detections are separated by 1.4" 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 | ATO J114.8607-22.9042 | 07:39:24.87 -22:54:34.2 (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 J114.8607-22.9042,2461061.5883,11.29,0.05,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
ATO J114.8607-22.9042 20260121.0883 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:23.95 -22:54:25.0 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 11.43 07:32:18.05 -20:32:12.7
235.76058 -0.69624 galactic Pup Second-epoch detections are separated by 1.4" 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 | Gaia DR3 5620193821859991552 | 07:32:18.11 -20:32:06.5 (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 5620193821859991552,2461061.5883,11.43,0.05,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 5620193821859991552 20260121.0883 11.43CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:32:18.05 -20:32:12.7 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 11.48 07:23:08.70 -21:47:31.5
235.84813 -3.17090 galactic CMa Second-epoch detections are separated by 1.6" 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 5619716736881376768 | 07:23:08.63 -21:47:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.266+/-0.035 (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 5619716736881376768,2461061.5883,11.48,0.05,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 5619716736881376768 20260121.0883 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:23:08.70 -21:47:31.5 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 11.57 07:37:18.75 -21:24:09.1
237.08556 -0.09407 galactic Pup Second-epoch detections are separated by 2.7" 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 | ATO J114.3206-21.3943 | 07:37:19.08 -21:24:15.6 (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 J114.3206-21.3943,2461061.5883,11.57,0.05,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
ATO J114.3206-21.3943 20260121.0883 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:18.75 -21:24:09.1 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 10.35 07:33:29.46 -21:08:10.6
236.41979 -0.74238 galactic Pup Second-epoch detections are separated by 0.4" 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 5620080572159093760 | 07:33:29.56 -21:08:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.649+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5620080572159093760,2461061.5883,10.35,0.05,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 5620080572159093760 20260121.0883 10.35CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:29.46 -21:08:10.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 11.35 07:18:02.35 -22:47:09.2
236.17816 -4.67893 galactic CMa 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 | Gaia DR3 5618179379120529792 | 07:18:02.39 -22:47:08.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.368+/-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
Gaia DR3 5618179379120529792,2461061.5883,11.35,0.05,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 5618179379120529792 20260121.0883 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:18:02.35 -22:47:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 10.29 06:40:46.88 -13:02:26.0
223.42083 -8.23245 galactic CMa Second-epoch detections are separated by 0.4" 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 J100.1891-13.0418 | 06:40:46.92 -13:02:26.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3II/III 1988MSS...C04....0H HD 48019 J-Ks=0.163+/-0.035 (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 J100.1891-13.0418,2461061.5883,10.29,0.05,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 J100.1891-13.0418 20260121.0883 10.29CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:46.88 -13:02:26.0 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0883 2461061.5883 10.36 07:27:05.60 -22:44:05.2
237.11210 -2.81056 galactic CMa Second-epoch detections are separated by 0.4" 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 5618661892925819008 | 07:27:05.73 -22:44:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.234+/-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 5618661892925819008,2461061.5883,10.36,0.05,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 5618661892925819008 20260121.0883 10.36CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20.00sec_-15.00C_LIGHT_0046.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMa-02-Q1b1x1_222120_TTUQ1b1x1_6729_TZJb8W6B/fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20.00sec_-14.90C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:27:05.60 -22:44:05.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-07-18_20_00sec_-14_90C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-20_20-06-35_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2338 2461061.7338 11.86 09:45:43.81 -13:15:59.9
248.81581 29.50096 galactic Hya Second-epoch detections are separated by 0.4" 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 5690528992264720512 | 09:45:42.84 -13:15:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.341+/-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 5690528992264720512,2461061.7338,11.86,0.05,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 5690528992264720512 20260121.2338 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/Sex-03-Q1b1x1_2025-12-23_03-51-09_20.00sec_-14.90C_LIGHT_0518.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Sex-03-Q1b1x1_002321_TTUQ1b1x1_7334_mKLPxTOm/fd_Sex-03-Q1b1x1_2026-01-20_23-36-12_20.00sec_-15.00C_LIGHT_0254.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Sex-03-Q1b1x1_002321_TTUQ1b1x1_7334_mKLPxTOm/fd_Sex-03-Q1b1x1_2026-01-20_23-36-50_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:45:43.81 -13:15:59.9 ;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_Sex-03-Q1b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q1b1x1_2026-01-20_23-36-50_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-03-Q1b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q1b1x1_2026-01-20_23-36-12_20_00sec_-15_00C_LIGHT_0254_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-03-Q1b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q1b1x1_2026-01-20_23-36-50_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-03-Q1b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q1b1x1_2026-01-20_23-36-12_20_00sec_-15_00C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2102 2461061.7102 13.62 08:22:10.66 -13:37:21.6
235.92679 13.07249 galactic Pup Second-epoch detections are separated by 1.5" 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 J125.5435-13.6216 | 08:22:10.66 -13:37:21.6 (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 J125.5435-13.6216,2461061.7102,13.62,0.05,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
ATO J125.5435-13.6216 20260121.2102 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/Hya-07-Q1b1x1_2025-12-23_02-18-00_20.00sec_-15.10C_LIGHT_0421.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_002937_TTUQ1b1x1_12443_CQpBGa9l/fd_Hya-07-Q1b1x1_2026-01-20_23-02-11_20.00sec_-15.00C_LIGHT_0219.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_002937_TTUQ1b1x1_12443_CQpBGa9l/fd_Hya-07-Q1b1x1_2026-01-20_23-02-58_20.00sec_-14.90C_LIGHT_0220.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:22:10.66 -13:37:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-20_23-02-58_20_00sec_-14_90C_LIGHT_0220_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-20_23-02-11_20_00sec_-15_00C_LIGHT_0219_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-20_23-02-58_20_00sec_-14_90C_LIGHT_0220_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-20_23-02-11_20_00sec_-15_00C_LIGHT_0219_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1958 2461061.6958 12.46 03:28:59.05 +37:19:28.7
154.54256 -15.69493 galactic Per 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 | Gaia DR3 222748965456232320 | 03:28:58.88 +37:19:28.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.585+/-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!
TCP 2026 01 21.1959* 03 28 59.05 +37 19 28.7 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 222748965456232320,2461061.6958,12.46,0.05,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 222748965456232320 20260121.1958 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/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Per-04-Q1b1x1_230944_TTUQ1b1x1_14985_npu2Rzwh/fd_Per-04-Q1b1x1_2026-01-20_22-41-27_20.00sec_-15.00C_LIGHT_0199.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Per-04-Q1b1x1_230944_TTUQ1b1x1_14985_npu2Rzwh/fd_Per-04-Q1b1x1_2026-01-20_22-42-15_20.00sec_-15.00C_LIGHT_0200.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:59.05 +37:19:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-01-20_22-42-15_20_00sec_-15_00C_LIGHT_0200_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-01-20_22-41-27_20_00sec_-15_00C_LIGHT_0199_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-01-20_22-42-15_20_00sec_-15_00C_LIGHT_0200_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-01-20_22-41-27_20_00sec_-15_00C_LIGHT_0199_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2139 2461061.7139 14.41 07:13:51.21 +03:52:27.7
212.02547 6.74897 galactic CMi Second-epoch detections are separated by 0.2" 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 J108.4638+03.8750 | 07:13:51.21 +03:52:27.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.4638+03.8750,2461061.7139,14.41,0.05,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
ATO J108.4638+03.8750 20260121.2139 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/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-07-22_20.00sec_-14.90C_LIGHT_0225.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20.00sec_-14.90C_LIGHT_0226.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:13:51.21 +03:52:27.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_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_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7139,12.31,0.05,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
target 20260121.2139 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/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-07-22_20.00sec_-14.90C_LIGHT_0225.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20.00sec_-14.90C_LIGHT_0226.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:59.36 +08:44:10.1 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_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_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7139,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.2139 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-07-22_20.00sec_-14.90C_LIGHT_0225.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20.00sec_-14.90C_LIGHT_0226.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:21:50.28 +00:40:23.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_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_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2139 2461061.7139 14.49 07:17:35.79 +10:38:44.2
206.30877 10.59423 galactic CMi Second-epoch detections are separated by 2.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.3990+10.6451 | 07:17:35.79 +10:38:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.992+/-0.136 (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 J109.3990+10.6451,2461061.7139,14.49,0.05,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 J109.3990+10.6451 20260121.2139 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_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-07-22_20.00sec_-14.90C_LIGHT_0225.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20.00sec_-14.90C_LIGHT_0226.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:17:35.79 +10:38:44.2 ;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_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_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_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7139,14.48,0.05,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
target 20260121.2139 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-07-22_20.00sec_-14.90C_LIGHT_0225.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20.00sec_-14.90C_LIGHT_0226.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:38:25.81 +05:48:58.1 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_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_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2139 2461061.7139 14.42 07:18:39.56 +03:40:50.7
212.74611 7.73063 galactic CMi Second-epoch detections are separated by 4.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.6570+03.6867 | 07:18:37.99 +03:41:27.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.162+/-0.229 (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 J109.6570+03.6867,2461061.7139,14.42,0.05,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
ATO J109.6570+03.6867 20260121.2139 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/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-07-22_20.00sec_-14.90C_LIGHT_0225.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_CMi-01-Q1b1x1_235520_TTUQ1b1x1_11017_C2OzQjr9/fd_CMi-01-Q1b1x1_2026-01-20_23-08-13_20.00sec_-14.90C_LIGHT_0226.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:18:39.56 +03:40:50.7 ;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_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_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_2026-01-20_23-08-13_20_00sec_-14_90C_LIGHT_0226_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_2026-01-20_23-07-22_20_00sec_-14_90C_LIGHT_0225_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1448 2461061.6448 14.40 01:02:41.86 +21:01:02.7
126.45628 -41.77727 galactic Psc Second-epoch detections are separated by 0.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:02:41.86 +21:01:02.7 (user input) | T | P | (position from user input) J-Ks=0.752+/-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
target,2461061.6448,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.1448 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/And-07-Q1b1x1_2025-12-22_22-13-09_20.00sec_-14.90C_LIGHT_0159.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_And-07-Q1b1x1_232321_TTUQ1b1x1_8270_EZKUoydC/fd_And-07-Q1b1x1_2026-01-20_21-27-55_20.00sec_-15.00C_LIGHT_0126.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_And-07-Q1b1x1_232321_TTUQ1b1x1_8270_EZKUoydC/fd_And-07-Q1b1x1_2026-01-20_21-28-45_20.00sec_-15.00C_LIGHT_0127.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:02:41.86 +21:01:02.7 ;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_And-07-Q1b1x1_2025-12-22_22-13-09_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_And-07-Q1b1x1_2026-01-20_21-28-45_20_00sec_-15_00C_LIGHT_0127_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-07-Q1b1x1_2025-12-22_22-13-09_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_And-07-Q1b1x1_2026-01-20_21-27-55_20_00sec_-15_00C_LIGHT_0126_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-07-Q1b1x1_2025-12-22_22-13-09_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_And-07-Q1b1x1_2026-01-20_21-28-45_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-07-Q1b1x1_2025-12-22_22-13-09_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_And-07-Q1b1x1_2026-01-20_21-27-55_20_00sec_-15_00C_LIGHT_0126_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.1434* 23 22 44.50 +39 32 50.9 13.1 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,2461061.6434,13.12,0.05,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 20260121.1434 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/And-04-Q1b1x1_2025-12-22_21-39-44_20.00sec_-15.00C_LIGHT_0127.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_And-04-Q1b1x1_230317_TTUQ1b1x1_8030_2m9DSSIR/fd_And-04-Q1b1x1_2026-01-20_21-25-53_20.00sec_-15.00C_LIGHT_0124.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_And-04-Q1b1x1_230317_TTUQ1b1x1_8030_2m9DSSIR/fd_And-04-Q1b1x1_2026-01-20_21-26-51_20.00sec_-15.00C_LIGHT_0125.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:44.50 +39:32:50.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-20_21-26-51_20_00sec_-15_00C_LIGHT_0125_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_2026-01-20_21-25-53_20_00sec_-15_00C_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_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-20_21-26-51_20_00sec_-15_00C_LIGHT_0125_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_2026-01-20_21-25-53_20_00sec_-15_00C_LIGHT_0124_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1434 2461061.6434 13.79 00:36:18.24 +40:19:34.0
119.81160 -22.45393 galactic And Second-epoch detections are separated by 0.1" 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 varaible 380801867868485376 | 00:36:18.24 +40:19:34.0 (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') SpType: K0 (LAMOST DR5) J-Ks=0.540+/-0.054 (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 21.1434* 00 36 18.24 +40 19 34.0 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 varaible 380801867868485376,2461061.6434,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 varaible 380801867868485376 20260121.1434 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_And-04-Q1b1x1_230317_TTUQ1b1x1_8030_2m9DSSIR/fd_And-04-Q1b1x1_2026-01-20_21-25-53_20.00sec_-15.00C_LIGHT_0124.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_And-04-Q1b1x1_230317_TTUQ1b1x1_8030_2m9DSSIR/fd_And-04-Q1b1x1_2026-01-20_21-26-51_20.00sec_-15.00C_LIGHT_0125.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:18.24 +40:19:34.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-20_21-26-51_20_00sec_-15_00C_LIGHT_0125_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_2026-01-20_21-25-53_20_00sec_-15_00C_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_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-20_21-26-51_20_00sec_-15_00C_LIGHT_0125_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_2026-01-20_21-25-53_20_00sec_-15_00C_LIGHT_0124_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1434 2461061.6434 14.36 23:48:57.71 +36:41:29.8
109.20626 -24.50937 galactic And Second-epoch detections are separated by 2.6" 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 | Gaia DR3 2879601853427469696 | 23:48:58.58 +36:40:50.8 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.452+/-0.059 (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 21.1434* 23 48 57.71 +36 41 29.8 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
Gaia DR3 2879601853427469696,2461061.6434,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2879601853427469696 20260121.1434 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_And-04-Q1b1x1_230317_TTUQ1b1x1_8030_2m9DSSIR/fd_And-04-Q1b1x1_2026-01-20_21-25-53_20.00sec_-15.00C_LIGHT_0124.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_And-04-Q1b1x1_230317_TTUQ1b1x1_8030_2m9DSSIR/fd_And-04-Q1b1x1_2026-01-20_21-26-51_20.00sec_-15.00C_LIGHT_0125.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:48:57.71 +36:41:29.8 ;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_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-20_21-26-51_20_00sec_-15_00C_LIGHT_0125_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_2026-01-20_21-25-53_20_00sec_-15_00C_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_And-04-Q1b1x1_2025-12-22_21-39-44_20_00sec_-15_00C_LIGHT_0127_fits__*pix.png resample_wcs_fd_And-04-Q1b1x1_2026-01-20_21-26-51_20_00sec_-15_00C_LIGHT_0125_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_2026-01-20_21-25-53_20_00sec_-15_00C_LIGHT_0124_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1166 2461061.6166 14.45 02:10:54.50 -22:31:41.9
202.97130 -71.41457 galactic Cet Second-epoch detections are separated by 3.4" 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 J032.7264-22.5283 | 02:10:54.50 -22:31:41.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.138+/-0.066 (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 21.1166* 02 10 54.50 -22 31 41.9 14.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J032.7264-22.5283,2461061.6166,14.45,0.05,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 J032.7264-22.5283 20260121.1166 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/Cet-11-Q1b1x1_2025-12-22_20-39-04_20.00sec_-14.90C_LIGHT_0061.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cet-11-Q1b1x1_221327_TTUQ1b1x1_29910_TZFQmoa4/fd_Cet-11-Q1b1x1_2026-01-20_20-47-17_20.00sec_-14.90C_LIGHT_0086.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cet-11-Q1b1x1_221327_TTUQ1b1x1_29910_TZFQmoa4/fd_Cet-11-Q1b1x1_2026-01-20_20-48-09_20.00sec_-14.90C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:10:54.50 -22:31:41.9 ;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_Cet-11-Q1b1x1_2025-12-22_20-39-04_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Cet-11-Q1b1x1_2026-01-20_20-48-09_20_00sec_-14_90C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-11-Q1b1x1_2025-12-22_20-39-04_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Cet-11-Q1b1x1_2026-01-20_20-47-17_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-11-Q1b1x1_2025-12-22_20-39-04_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Cet-11-Q1b1x1_2026-01-20_20-48-09_20_00sec_-14_90C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-11-Q1b1x1_2025-12-22_20-39-04_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Cet-11-Q1b1x1_2026-01-20_20-47-17_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7314,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.2314 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Cam-09-Q1b1x1_011724_TTUQ1b1x1_17931_hqf23b2d/fd_Cam-09-Q1b1x1_2026-01-20_23-32-38_20.00sec_-15.00C_LIGHT_0250.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-09-Q1b1x1_011724_TTUQ1b1x1_17931_hqf23b2d/fd_Cam-09-Q1b1x1_2026-01-20_23-33-23_20.00sec_-14.90C_LIGHT_0251.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:43.00 +59:34:27.6 ;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_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-20_23-33-23_20_00sec_-14_90C_LIGHT_0251_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_2026-01-20_23-32-38_20_00sec_-15_00C_LIGHT_0250_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_2026-01-20_23-33-23_20_00sec_-14_90C_LIGHT_0251_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_2026-01-20_23-32-38_20_00sec_-15_00C_LIGHT_0250_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0570 2461061.5570 14.36 21:58:03.47 +53:02:01.3
98.54571 -1.42578 galactic Cyg Second-epoch detections are separated by 1.6" 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 J329.5154+53.0298 | 21:58:03.47 +53:02:01.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.557+/-0.130 (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 J329.5154+53.0298,2461061.5570,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J329.5154+53.0298 20260121.0570 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Cyg-02-Q1b1x1_204848_TTUQ1b1x1_25119_DpvNTDRs/fd_Cyg-02-Q1b1x1_2026-01-20_19-21-35_20.00sec_-15.00C_LIGHT_0006.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-02-Q1b1x1_204848_TTUQ1b1x1_25119_DpvNTDRs/fd_Cyg-02-Q1b1x1_2026-01-20_19-22-18_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:03.47 +53:02:01.3 ;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_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-20_19-22-18_20_00sec_-15_00C_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_2026-01-20_19-21-35_20_00sec_-15_00C_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_2026-01-20_19-22-18_20_00sec_-15_00C_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_2026-01-20_19-21-35_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0570 2461061.5570 13.76 21:43:14.29 +53:09:51.9
96.90340 0.08020 galactic Cyg Second-epoch detections are separated by 0.4" 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 J325.8093+53.1646 | 21:43:14.29 +53:09:51.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.440+/-0.053 (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 J325.8093+53.1646,2461061.5570,13.76,0.05,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 J325.8093+53.1646 20260121.0570 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/Cyg-02-Q1b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-02-Q1b1x1_204848_TTUQ1b1x1_25119_DpvNTDRs/fd_Cyg-02-Q1b1x1_2026-01-20_19-21-35_20.00sec_-15.00C_LIGHT_0006.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-02-Q1b1x1_204848_TTUQ1b1x1_25119_DpvNTDRs/fd_Cyg-02-Q1b1x1_2026-01-20_19-22-18_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:43:14.29 +53:09:51.9 ;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_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-20_19-22-18_20_00sec_-15_00C_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_2026-01-20_19-21-35_20_00sec_-15_00C_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_2026-01-20_19-22-18_20_00sec_-15_00C_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_2026-01-20_19-21-35_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0570 2461061.5570 14.39 21:54:29.76 +53:51:58.3
98.64078 -0.44334 galactic Cyg Second-epoch detections are separated by 1.7" 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 J328.6256+53.8735 | 21:54:30.16 +53:52:24.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.449+/-0.109 (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 J328.6256+53.8735,2461061.5570,14.39,0.05,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
ATO J328.6256+53.8735 20260121.0570 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/Cyg-02-Q1b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-02-Q1b1x1_204848_TTUQ1b1x1_25119_DpvNTDRs/fd_Cyg-02-Q1b1x1_2026-01-20_19-21-35_20.00sec_-15.00C_LIGHT_0006.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cyg-02-Q1b1x1_204848_TTUQ1b1x1_25119_DpvNTDRs/fd_Cyg-02-Q1b1x1_2026-01-20_19-22-18_20.00sec_-15.00C_LIGHT_0007.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:54:29.76 +53:51:58.3 ;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_Cyg-02-Q1b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q1b1x1_2026-01-20_19-22-18_20_00sec_-15_00C_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_2026-01-20_19-21-35_20_00sec_-15_00C_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_2026-01-20_19-22-18_20_00sec_-15_00C_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_2026-01-20_19-21-35_20_00sec_-15_00C_LIGHT_0006_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0981 2461061.5981 14.40 07:03:47.91 +13:59:10.7
201.76644 9.01894 galactic Gem Second-epoch detections are separated by 0.2" 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 J105.9507+13.9878 | 07:03:47.25 +13:58:31.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.364+/-0.064 (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 J105.9507+13.9878,2461061.5981,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9507+13.9878 20260121.0981 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-20-31_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:03:47.91 +13:59:10.7 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0981 2461061.5981 14.33 06:49:18.38 +09:49:59.0
203.92522 3.99768 galactic Mon Second-epoch detections are separated by 3.9" 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 3158499914186542336 | 06:49:21.26 +09:50:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3158499914186542336,2461061.5981,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3158499914186542336 20260121.0981 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-20-31_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:49:18.38 +09:49:59.0 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0981 2461061.5981 13.33 06:42:12.39 +13:25:59.8
199.91818 4.07560 galactic Gem Second-epoch detections are separated by 1.4" 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 3352760705166560000 | 06:42:10.38 +13:26:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3352760705166560000,2461061.5981,13.33,0.05,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 3352760705166560000 20260121.0981 13.33CV 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/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-20-31_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:42:12.39 +13:25:59.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0981 2461061.5981 14.27 06:54:14.87 +11:10:37.6
203.26854 5.68697 galactic Mon Second-epoch detections are separated by 5.7" 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 | ATO J103.5630+11.1787 | 06:54:14.87 +11:10:37.6 (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 J103.5630+11.1787,2461061.5981,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.5630+11.1787 20260121.0981 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-20-31_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:54:14.87 +11:10:37.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5981,14.22,0.05,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 20260121.0981 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/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-20-31_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:54:12.96 +16:16:14.5 ;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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0981 2461061.5981 14.31 06:45:42.20 +15:48:56.5
198.16491 5.90341 galactic Gem 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 | target | 06:45:42.20 +15:48:56.5 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.059 (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,2461061.5981,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.0981 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/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-20-31_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:45:42.20 +15:48:56.5 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5981,14.46,0.05,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
target 20260121.0981 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/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-20-31_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:39:48.42 +12:16:37.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0981 2461061.5981 14.45 07:00:41.27 +17:08:52.9
198.54983 9.71556 galactic Gem Second-epoch detections are separated by 3.5" 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 | target | 07:00:41.27 +17:08:52.9 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5981,14.45,0.05,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 20260121.0981 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/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-20-31_20.00sec_-15.00C_LIGHT_0058.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-05-Q1b1x1_213232_TTUQ1b1x1_20972_T2iswWBs/fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:41.27 +17:08:52.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_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_2026-01-20_20-21-34_20_00sec_-15_00C_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_2026-01-20_20-20-31_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3120 2461061.8120 11.91 18:15:44.06 +61:57:03.0
91.23329 27.86299 galactic Dra Second-epoch detections are separated by 0.9" 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 2159110094405704064 | 18:15:44.13 +61:57:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-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 2159110094405704064,2461061.8120,11.91,0.05,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 2159110094405704064 20260121.3120 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/Dra-07-Q1b1x1_2025-12-23_06-37-17_20.00sec_-15.00C_LIGHT_0702.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-07-Q1b1x1_013114_TTUQ1b1x1_17547_5LLfCN8y/fd_Dra-07-Q1b1x1_2026-01-21_01-28-41_20.00sec_-15.00C_LIGHT_0347.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-07-Q1b1x1_013114_TTUQ1b1x1_17547_5LLfCN8y/fd_Dra-07-Q1b1x1_2026-01-21_01-29-33_20.00sec_-15.00C_LIGHT_0348.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:15:44.06 +61:57:03.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-07-Q1b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q1b1x1_2026-01-21_01-29-33_20_00sec_-15_00C_LIGHT_0348_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_2026-01-21_01-28-41_20_00sec_-15_00C_LIGHT_0347_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_2026-01-21_01-29-33_20_00sec_-15_00C_LIGHT_0348_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_2026-01-21_01-28-41_20_00sec_-15_00C_LIGHT_0347_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3120 2461061.8120 11.94 17:25:32.95 +56:58:34.7
85.19180 34.04631 galactic Dra Second-epoch detections are separated by 0.5" 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 | Gaia DR3 1420858984919444480 | 17:25:33.02 +56:58:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.420+/-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
Gaia DR3 1420858984919444480,2461061.8120,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1420858984919444480 20260121.3120 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Dra-07-Q1b1x1_013114_TTUQ1b1x1_17547_5LLfCN8y/fd_Dra-07-Q1b1x1_2026-01-21_01-28-41_20.00sec_-15.00C_LIGHT_0347.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-07-Q1b1x1_013114_TTUQ1b1x1_17547_5LLfCN8y/fd_Dra-07-Q1b1x1_2026-01-21_01-29-33_20.00sec_-15.00C_LIGHT_0348.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:32.95 +56:58:34.7 ;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_Dra-07-Q1b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q1b1x1_2026-01-21_01-29-33_20_00sec_-15_00C_LIGHT_0348_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_2026-01-21_01-28-41_20_00sec_-15_00C_LIGHT_0347_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_2026-01-21_01-29-33_20_00sec_-15_00C_LIGHT_0348_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_2026-01-21_01-28-41_20_00sec_-15_00C_LIGHT_0347_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2445 2461061.7445 12.51 08:51:44.14 +11:46:30.7
215.77516 31.98269 galactic Cnc Second-epoch detections are separated by 1.2" 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 604916731706106752 | 08:51:42.67 +11:46:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1940ApJ....91..244E NGC 2682 221
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 604916731706106752,2461061.7445,12.51,0.05,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 604916731706106752 20260121.2445 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Cnc-05-Q1b1x1_015558_TTUQ1b1x1_16246_QaL4gtZt/fd_Cnc-05-Q1b1x1_2026-01-20_23-51-33_20.00sec_-15.00C_LIGHT_0271.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cnc-05-Q1b1x1_015558_TTUQ1b1x1_16246_QaL4gtZt/fd_Cnc-05-Q1b1x1_2026-01-20_23-52-16_20.00sec_-15.00C_LIGHT_0272.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:51:44.14 +11:46:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q1b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q1b1x1_2026-01-20_23-52-16_20_00sec_-15_00C_LIGHT_0272_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_2026-01-20_23-51-33_20_00sec_-15_00C_LIGHT_0271_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_2026-01-20_23-52-16_20_00sec_-15_00C_LIGHT_0272_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_2026-01-20_23-51-33_20_00sec_-15_00C_LIGHT_0271_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 8.21 11:13:39.46 -22:59:39.0
275.36794 34.59058 galactic Crt Second-epoch detections are separated by 0.9" 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 | HIP 54843 | 11:13:40.94 -22:59:55.4 (Gaia DR3) | VAR (local) | 0.114130000000 (local) | Gaia3var=NOT_AVAILABLE SpType: A8V 1988MSS...C04....0H HD 97590
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HIP 54843,2461061.7362,8.21,0.05,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
HIP 54843 20260121.2362 8.21CV 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-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:39.46 -22:59:39.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 12.03 11:13:27.30 -22:53:09.0
275.25826 34.66653 galactic Crt 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 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 3538071638994004864,2461061.7362,12.03,0.05,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 3538071638994004864 20260121.2362 12.03CV 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-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:27.30 -22:53:09.0 ;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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 12.47 11:10:58.50 -23:05:09.7
274.75105 34.22960 galactic Crt 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 3537962993501377024 | 11:10:58.91 -23:05:14.5 (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 3537962993501377024,2461061.7362,12.47,0.05,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 3537962993501377024 20260121.2362 12.47CV 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_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:10:58.50 -23:05:09.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 12.63 10:52:28.39 -21:51:17.8
269.55047 33.19378 galactic Hya Second-epoch detections are separated by 0.4" 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 | target | 10:52:28.39 -21:51:17.8 (user input) | T | P | (position from user input) J-Ks=0.310+/-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,2461061.7362,12.63,0.05,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
target 20260121.2362 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:52:28.39 -21:51:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 12.65 10:53:36.56 -23:07:32.4
270.60569 32.24747 galactic Hya Second-epoch detections are separated by 8.2" 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 3549080185633326976 | 10:53:37.11 -23:07:29.9 (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 3549080185633326976,2461061.7362,12.65,0.05,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 3549080185633326976 20260121.2362 12.65CV 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:53:36.56 -23:07:32.4 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 12.57 11:13:37.44 -23:03:07.5
275.39099 34.53532 galactic Crt Second-epoch detections are separated by 2.1" 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 | Gaia DR3 3537928839921612800 | 11:13:38.96 -23:03:27.4 (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 3537928839921612800,2461061.7362,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3537928839921612800 20260121.2362 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:37.44 -23:03:07.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 12.68 11:10:42.25 -23:04:36.0
274.67888 34.20943 galactic Crt Second-epoch detections are separated by 2.5" 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 3537963611976665600 | 11:10:42.59 -23:04:40.0 (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 3537963611976665600,2461061.7362,12.68,0.05,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 3537963611976665600 20260121.2362 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:10:42.25 -23:04:36.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7362,13.26,0.05,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 20260121.2362 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:09:10.55 -19:06:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 13.18 11:11:30.54 -18:17:23.0
272.09640 38.52587 galactic Crt Second-epoch detections are separated by 7.2" 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 | Large-amplitude variable Gaia DR2 3558205243086603520 | 11:11:30.54 -18:17:23.0 (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=1.193+/-0.097 (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 3558205243086603520,2461061.7362,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3558205243086603520 20260121.2362 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:11:30.54 -18:17:23.0 ;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-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 13.57 10:53:40.57 -21:47:33.7
269.79544 33.39353 galactic Hya Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J163.4187-21.7929 | 10:53:40.57 -21:47:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.197+/-0.165 (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 J163.4187-21.7929,2461061.7362,13.57,0.05,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 J163.4187-21.7929 20260121.2362 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:53:40.57 -21:47:33.7 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 12.41 10:50:57.91 -22:09:20.1
269.38665 32.75370 galactic Hya Second-epoch detections are separated by 1.6" 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 | Gaia DR3 3550145200083113600 | 10:50:57.95 -22:09:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.478+/-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 3550145200083113600,2461061.7362,12.41,0.05,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 3550145200083113600 20260121.2362 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/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_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:50:57.91 -22:09:20.1 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 13.01 11:08:13.52 -19:52:29.2
272.20280 36.76316 galactic Crt Second-epoch detections are separated by 0.4" 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 | target | 11:08:13.52 -19:52:29.2 (user input) | T | P | (position from user input) J-Ks=0.741+/-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
target,2461061.7362,13.01,0.05,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 20260121.2362 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/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_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:08:13.52 -19:52:29.2 ;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-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2362 2461061.7362 11.39 11:01:14.38 -20:06:16.4
270.57603 35.75040 galactic Crt 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 | Gaia DR3 3551604153230007296 | 11:01:14.35 -20:06:15.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.999+/-0.040 (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 3551604153230007296,2461061.7362,11.39,0.05,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 3551604153230007296 20260121.2362 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/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_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-39-30_20.00sec_-15.00C_LIGHT_0258.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_003341_TTUQ1b1x1_17414_NOWiEplB/fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20.00sec_-14.90C_LIGHT_0259.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:01:14.38 -20:06:16.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_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_2026-01-20_23-40-29_20_00sec_-14_90C_LIGHT_0259_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_2026-01-20_23-39-30_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0652 2461061.5652 14.45 00:57:53.84 +59:59:39.9
123.74041 -2.86719 galactic Cas Second-epoch detections are separated by 1.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426082475423108096 | 00:57:48.90 +59:59:57.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G8 1935BSD...C01....0S BSD 8- 399
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.0652* 00 57 53.84 +59 59 39.9 14.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426082475423108096,2461061.5652,14.45,0.05,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
Gaia DR3 426082475423108096 20260121.0652 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:57:53.84 +59:59:39.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0652 2461061.5652 13.72 00:07:35.23 +62:20:32.1
117.86755 -0.09754 galactic Cas Second-epoch detections are separated by 0.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 429967565390645376 | 00:07:32.09 +62:19:54.2 (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 21.0652* 00 07 35.23 +62 20 32.1 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 429967565390645376,2461061.5652,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 429967565390645376 20260121.0652 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:07:35.23 +62:20:32.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.0652* 00 16 10.60 +64 11 53.4 14.3 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
target,2461061.5652,14.34,0.05,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 20260121.0652 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:16:10.60 +64:11:53.4 ;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_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5652,14.41,0.05,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
target 20260121.0652 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:55:38.94 +63:18:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.0652* 23 22 20.32 +60 37 21.0 14.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5652,14.46,0.05,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
target 20260121.0652 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:22:20.32 +60:37:21.0 ;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_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0652 2461061.5652 14.46 00:56:38.78 +60:27:34.4
123.57443 -2.40570 galactic Cas Second-epoch detections are separated by 1.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:56:38.78 +60:27:34.4 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.081 (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 21.0652* 00 56 38.78 +60 27 34.4 14.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5652,14.46,0.05,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
target 20260121.0652 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:56:38.78 +60:27:34.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.0652 2461061.5652 14.37 00:12:08.85 +57:26:46.9
117.64457 -5.02148 galactic Cas Second-epoch detections are separated by 2.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:12:08.85 +57:26:46.9 (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 21.0652* 00 12 08.85 +57 26 46.9 14.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5652,14.37,0.05,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 20260121.0652 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/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:12:08.85 +57:26:46.9 ;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_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.0652* 00 58 25.51 +61 06 30.9 14.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.5652,14.48,0.05,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
target 20260121.0652 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-22_22-20-50_20.00sec_-14.90C_LIGHT_0168.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20.00sec_-14.90C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cas-02-Q1b1x1_203235_TTUQ1b1x1_6297_wpu9tsLk/fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:58:25.51 +61:06:30.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-34-13_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-02-Q1b1x1_2025-12-22_22-20-50_20_00sec_-14_90C_LIGHT_0168_fits__*pix.png resample_wcs_fd_Cas-02-Q1b1x1_2026-01-20_19-33-13_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2115 2461061.7115 14.09 08:11:13.85 -11:14:57.3
232.41643 12.05510 galactic Hya Second-epoch detections are separated by 5.1" 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 | ATO J122.8028-11.2566 | 08:11:13.85 -11:14:57.3 (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 J122.8028-11.2566,2461061.7115,14.09,0.05,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
ATO J122.8028-11.2566 20260121.2115 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Hya-05-Q1b1x1_001917_TTUQ1b1x1_21239_iWOPp41W/fd_Hya-05-Q1b1x1_2026-01-20_23-03-59_20.00sec_-14.90C_LIGHT_0221.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-05-Q1b1x1_001917_TTUQ1b1x1_21239_iWOPp41W/fd_Hya-05-Q1b1x1_2026-01-20_23-04-50_20.00sec_-14.90C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:13.85 -11:14:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-20_23-04-50_20_00sec_-14_90C_LIGHT_0222_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_2026-01-20_23-03-59_20_00sec_-14_90C_LIGHT_0221_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_2026-01-20_23-04-50_20_00sec_-14_90C_LIGHT_0222_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_2026-01-20_23-03-59_20_00sec_-14_90C_LIGHT_0221_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 12.75 07:54:23.24 +24:35:25.7
196.51383 24.15743 galactic Gem Second-epoch detections are separated by 0.3" 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 | target | 07:54:23.24 +24:35:25.7 (user input) | T | P | (position from user input) J-Ks=0.397+/-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
target,2461061.7223,12.75,0.05,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 20260121.2223 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/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:54:23.24 +24:35:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 14.12 07:20:30.08 +22:26:09.3
195.58742 16.14481 galactic Gem Second-epoch detections are separated by 2.4" and 8.6 pix This object is listed in planets.txt 884.1" Jupiter (-2.7mag)
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 | 07:20:30.08 +22:26:09.3 (user input) | T | P | (position from user input) J-Ks=0.433+/-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
target,2461061.7223,14.12,0.05,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 20260121.2223 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/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:20:30.08 +22:26:09.3 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 14.20 07:46:54.53 +26:52:20.7
193.54260 23.35244 galactic Gem Second-epoch detections are separated by 0.5" 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 | Large-amplitude variable Gaia DR2 874938031366744704 | 07:46:54.53 +26:52:20.7 (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=0.934+/-0.069 (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 874938031366744704,2461061.7223,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 874938031366744704 20260121.2223 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:54.53 +26:52:20.7 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 11.66 07:55:12.69 +24:07:15.9
197.06770 24.17141 galactic Gem Second-epoch detections are separated by 0.4" 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 681456008155050496 | 07:55:12.70 +24:07:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.646+/-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
Gaia DR3 681456008155050496,2461061.7223,11.66,0.05,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
Gaia DR3 681456008155050496 20260121.2223 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/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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:55:12.69 +24:07:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 11.54 07:50:03.23 +25:40:26.1
195.03280 23.60796 galactic Gem Second-epoch detections are separated by 0.1" 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 J117.5234+25.6735 | 07:50:03.22 +25:40:26.1 (Gaia DR3) | CBF (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.343+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J117.5234+25.6735,2461061.7223,11.54,0.05,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 J117.5234+25.6735 20260121.2223 11.54CV 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/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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:03.23 +25:40:26.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 12.69 07:48:37.49 +26:49:16.5
193.73585 23.69556 galactic Gem Second-epoch detections are separated by 0.4" 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 | target | 07:48:37.49 +26:49:16.5 (user input) | T | P | (position from user input) J-Ks=0.604+/-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,2461061.7223,12.69,0.05,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
target 20260121.2223 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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:48:37.49 +26:49:16.5 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 13.65 07:44:42.55 +25:30:60.0
194.74031 22.42290 galactic Gem Second-epoch detections are separated by 2.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:44:42.55 +25:30:60.0 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.574+/-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,2461061.7223,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.2223 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:44:42.55 +25:30:60.0 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 13.03 07:47:10.42 +25:12:48.4
195.25872 22.83875 galactic Gem Second-epoch detections are separated by 0.4" 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 | 07:47:10.42 +25:12:48.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.352+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7223,13.03,0.05,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
target 20260121.2223 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/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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:47:10.42 +25:12:48.4 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 12.98 07:50:59.54 +24:08:56.9
196.67215 23.27909 galactic Gem Second-epoch detections are separated by 0.2" 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 | target | 07:50:59.54 +24:08:56.9 (user input) | T | P | (position from user input) J-Ks=0.596+/-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
target,2461061.7223,12.98,0.05,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
target 20260121.2223 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/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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:59.54 +24:08:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 12.22 07:49:04.78 +25:39:34.0
194.96560 23.39678 galactic Gem Second-epoch detections are separated by 0.4" 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 J117.2695+25.6549 | 07:49:04.76 +25:39:34.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.508+/-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 J117.2695+25.6549,2461061.7223,12.22,0.05,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 J117.2695+25.6549 20260121.2223 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-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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:49:04.78 +25:39:34.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 10.97 07:41:09.73 +26:49:30.9
193.11536 22.13180 galactic Gem Second-epoch detections are separated by 0.2" 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 869166523033656448 | 07:41:09.71 +26:49:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.190+/-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 869166523033656448,2461061.7223,10.97,0.05,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
Gaia DR3 869166523033656448 20260121.2223 10.97CV 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/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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:09.73 +26:49:30.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2223 2461061.7223 13.51 07:55:53.14 +25:15:45.7
195.94706 24.70606 galactic Gem 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 | target | 07:55:53.14 +25:15:45.7 (user input) | T | P | (position from user input) J-Ks=0.650+/-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
target,2461061.7223,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.2223 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:55:53.14 +25:15:45.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7223,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.2223 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-19-27_20.00sec_-15.00C_LIGHT_0237.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-04-Q1b1x1_233322_TTUQ1b1x1_7964_T0TyhBxx/fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:48:16.86 +24:18:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-20_23-20-29_20_00sec_-15_00C_LIGHT_0238_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_2026-01-20_23-19-27_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2897 2461061.7897 9.67 11:03:30.84 -39:01:16.7
281.01431 19.21368 galactic Ant Second-epoch detections are separated by 3.1" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 21.2897* 11 03 30.84 -39 01 16.7 9.7 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 5390795186164872448,2461061.7897,9.67,0.05,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 5390795186164872448 20260121.2897 9.67CV 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/Ant-02-Q1b1x1_2026-01-09_02-37-11_20.00sec_-15.00C_LIGHT_0014.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-02-Q1b1x1_020956_TTUQ1b1x1_20442_gCRtzcrh/fd_Ant-02-Q1b1x1_2026-01-21_00-56-38_20.00sec_-14.90C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-02-Q1b1x1_020956_TTUQ1b1x1_20442_gCRtzcrh/fd_Ant-02-Q1b1x1_2026-01-21_00-57-17_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:03:30.84 -39:01:16.7 ;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_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-21_00-57-17_20_00sec_-15_00C_LIGHT_0320_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_2026-01-21_00-56-38_20_00sec_-14_90C_LIGHT_0319_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_2026-01-21_00-57-17_20_00sec_-15_00C_LIGHT_0320_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_2026-01-21_00-56-38_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2897 2461061.7897 10.29 11:05:34.54 -38:53:05.4
281.33767 19.50729 galactic Ant Second-epoch detections are separated by 5.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 21.2897* 11 05 34.54 -38 53 05.4 10.3 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 5396793125172481280,2461061.7897,10.29,0.05,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 5396793125172481280 20260121.2897 10.29CV 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_2026-01-21_CI_Ant-02-Q1b1x1_020956_TTUQ1b1x1_20442_gCRtzcrh/fd_Ant-02-Q1b1x1_2026-01-21_00-56-38_20.00sec_-14.90C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-02-Q1b1x1_020956_TTUQ1b1x1_20442_gCRtzcrh/fd_Ant-02-Q1b1x1_2026-01-21_00-57-17_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:34.54 -38:53:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-02-Q1b1x1_2026-01-09_02-37-11_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png resample_wcs_fd_Ant-02-Q1b1x1_2026-01-21_00-57-17_20_00sec_-15_00C_LIGHT_0320_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_2026-01-21_00-56-38_20_00sec_-14_90C_LIGHT_0319_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_2026-01-21_00-57-17_20_00sec_-15_00C_LIGHT_0320_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_2026-01-21_00-56-38_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2296 2461061.7296 12.27 07:41:43.03 +18:03:41.1
201.85992 18.99676 galactic Gem Second-epoch detections are separated by 2.5" 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 671171348186868352 | 07:41:42.63 +18:03:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4IV 1950ApJ...112...48M HD 61787
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 671171348186868352,2461061.7296,12.27,0.05,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 671171348186868352 20260121.2296 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/Cnc-04-Q1b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-01_20.00sec_-15.00C_LIGHT_0248.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20.00sec_-15.00C_LIGHT_0249.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:43.03 +18:03:41.1 ;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_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_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_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7296,14.14,0.05,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
target 20260121.2296 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-04-Q1b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-01_20.00sec_-15.00C_LIGHT_0248.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20.00sec_-15.00C_LIGHT_0249.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:20:00.24 +17:08:57.1 ;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_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_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_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2296 2461061.7296 12.79 08:26:18.36 +18:35:27.9
205.71380 28.99047 galactic Cnc Second-epoch detections are separated by 1.3" 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 J126.5769+18.5911 | 08:26:18.36 +18:35:27.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.300+/-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 J126.5769+18.5911,2461061.7296,12.79,0.05,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 J126.5769+18.5911 20260121.2296 12.79CV 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/Cnc-04-Q1b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-01_20.00sec_-15.00C_LIGHT_0248.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20.00sec_-15.00C_LIGHT_0249.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:26:18.36 +18:35:27.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_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_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2296 2461061.7296 13.79 08:31:47.30 +15:32:29.0
209.50902 29.06061 galactic Cnc Second-epoch detections are separated by 0.9" 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 | target | 08:31:47.30 +15:32:29.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.299+/-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,2461061.7296,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.2296 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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/reference_imgs/Cnc-04-Q1b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-01_20.00sec_-15.00C_LIGHT_0248.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20.00sec_-15.00C_LIGHT_0249.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:31:47.30 +15:32:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_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_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2296 2461061.7296 12.43 08:30:30.51 +14:13:17.7
210.75420 28.25828 galactic Cnc 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 651650202134717824 | 08:30:30.56 +14:13:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.310+/-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 651650202134717824,2461061.7296,12.43,0.05,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
Gaia DR3 651650202134717824 20260121.2296 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/Cnc-04-Q1b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-01_20.00sec_-15.00C_LIGHT_0248.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cnc-04-Q1b1x1_234514_TTUQ1b1x1_28340_kHVGDzht/fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20.00sec_-15.00C_LIGHT_0249.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:30.51 +14:13:17.7 ;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_Cnc-04-Q1b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q1b1x1_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_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_2026-01-20_23-30-58_20_00sec_-15_00C_LIGHT_0249_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_2026-01-20_23-30-01_20_00sec_-15_00C_LIGHT_0248_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3506 2461061.8506 13.88 04:08:14.60 +41:28:57.6
157.83918 -7.67820 galactic Per Second-epoch detections are separated by 3.1" 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 | 04:08:14.60 +41:28:57.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3506* 04 08 14.60 +41 28 57.6 13.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8506,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3506 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2025-12-23_01-19-40_20.00sec_-14.90C_LIGHT_0370.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-03-Q1b1x1_022603_TTUQ1b1x1_8661_9clJ3eLF/fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20.00sec_-14.90C_LIGHT_0393.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-03-Q1b1x1_022603_TTUQ1b1x1_8661_9clJ3eLF/fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20.00sec_-15.00C_LIGHT_0394.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:08:14.60 +41:28:57.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20_00sec_-14_90C_LIGHT_0393_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20_00sec_-15_00C_LIGHT_0394_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20_00sec_-14_90C_LIGHT_0393_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3506 2461061.8506 14.13 04:51:19.15 +41:46:48.4
163.16265 -1.62301 galactic Aur Second-epoch detections are separated by 1.8" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J072.8274+41.7799 | 04:51:19.56 +41:47:30.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1949AnHar.112....1C HD 277008
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J072.8274+41.7799,2461061.8506,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J072.8274+41.7799 20260121.3506 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Per-03-Q1b1x1_2025-12-23_01-19-40_20.00sec_-14.90C_LIGHT_0370.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-03-Q1b1x1_022603_TTUQ1b1x1_8661_9clJ3eLF/fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20.00sec_-14.90C_LIGHT_0393.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-03-Q1b1x1_022603_TTUQ1b1x1_8661_9clJ3eLF/fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20.00sec_-15.00C_LIGHT_0394.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:19.15 +41:46:48.4 ;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_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20_00sec_-14_90C_LIGHT_0393_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20_00sec_-15_00C_LIGHT_0394_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20_00sec_-14_90C_LIGHT_0393_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3506 2461061.8506 14.41 04:48:00.97 +40:45:18.6
163.55235 -2.75618 galactic Per Second-epoch detections are separated by 2.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J044803.86+404501.2 | 04:48:03.86 +40:45:01.2 (Gaia DR3) | SR (local) | 484.000000000000 (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3506* 04 48 00.97 +40 45 18.6 14.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044803.86+404501.2,2461061.8506,14.41,0.05,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
ASASSN-V J044803.86+404501.2 20260121.3506 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/Per-03-Q1b1x1_2025-12-23_01-19-40_20.00sec_-14.90C_LIGHT_0370.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-03-Q1b1x1_022603_TTUQ1b1x1_8661_9clJ3eLF/fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20.00sec_-14.90C_LIGHT_0393.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-03-Q1b1x1_022603_TTUQ1b1x1_8661_9clJ3eLF/fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20.00sec_-15.00C_LIGHT_0394.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:48:00.97 +40:45:18.6 ;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_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20_00sec_-14_90C_LIGHT_0393_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-58_20_00sec_-15_00C_LIGHT_0394_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-03-Q1b1x1_2025-12-23_01-19-40_20_00sec_-14_90C_LIGHT_0370_fits__*pix.png resample_wcs_fd_Per-03-Q1b1x1_2026-01-21_02-24-20_20_00sec_-14_90C_LIGHT_0393_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3418 2461061.8418 14.49 04:50:50.68 +33:57:16.5
169.16481 -6.66618 galactic Aur Second-epoch detections are separated by 4.4" 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 161884704730002048 | 04:50:52.30 +33:57:42.6 (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 161884704730002048,2461061.8418,14.49,0.05,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
Gaia DR3 161884704730002048 20260121.3418 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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:50.68 +33:57:16.5 ;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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3419* 04 49 47.01 +28 19 47.4 14.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8418,14.46,0.05,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
target 20260121.3418 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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:47.01 +28:19:47.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 11.57 08:12:41.03 -21:33:26.2
241.46456 6.87960 galactic Pup 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 | Gaia DR3 5700706729031126656 | 08:12:40.90 -21:33:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M4 1985ApJS...59..197B LTT 3080
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5700706729031126656,2461061.7703,11.57,0.05,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 5700706729031126656 20260121.2703 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:12:41.03 -21:33:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 13.42 08:07:06.33 -29:53:28.2
247.81073 1.31261 galactic Pup Second-epoch detections are separated by 4.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J121.7849-29.8929 | 08:07:08.40 -29:53:51.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1968ArA.....4..587L NGC 2533 4
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J121.7849-29.8929,2461061.7703,13.42,0.05,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
ATO J121.7849-29.8929 20260121.2703 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:06.33 -29:53:28.2 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 13.44 08:07:04.67 -29:53:20.0
247.80557 1.30878 galactic Pup Second-epoch detections are separated by 3.4" 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 | NSV 17740 | 08:07:02.04 -29:53:48.7 (Gaia DR3) | VAR: (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: F8 1968ArA.....4..587L NGC 2533 11
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 17740,2461061.7703,13.44,0.05,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
NSV 17740 20260121.2703 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:04.67 -29:53:20.0 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 13.66 08:21:07.08 -30:46:00.9
250.21381 3.34825 galactic Pup Second-epoch detections are separated by 2.8" 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 | 08:21:07.08 -30:46:00.9 (user input) | T | P | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7703,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.2703 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:21:07.08 -30:46:00.9 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 13.77 08:10:49.21 -26:57:57.9
245.79324 3.58428 galactic Pup Second-epoch detections are separated by 2.4" 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 | ATO J122.7042-26.9668 | 08:10:47.67 -26:57:21.2 (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 J122.7042-26.9668,2461061.7703,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J122.7042-26.9668 20260121.2703 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:49.21 -26:57:57.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 13.78 08:23:33.55 -29:26:09.1
249.41667 4.53907 galactic Pup Second-epoch detections are separated by 0.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J125.8871-29.4347 | 08:23:33.55 -29:26:09.1 (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 J125.8871-29.4347,2461061.7703,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J125.8871-29.4347 20260121.2703 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:33.55 -29:26:09.1 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 13.77 08:29:56.54 -27:03:41.0
248.27551 7.05401 galactic Pyx Second-epoch detections are separated by 3.6" 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 J127.4973-27.0690 | 08:29:56.54 -27:03:41.0 (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 J127.4973-27.0690,2461061.7703,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J127.4973-27.0690 20260121.2703 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:56.54 -27:03:41.0 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 13.93 08:04:12.90 -23:57:15.6
242.44512 3.94631 galactic Pup Second-epoch detections are separated by 2.0" 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 J121.0546-23.9663 | 08:04:12.90 -23:57:15.6 (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 J121.0546-23.9663,2461061.7703,13.93,0.05,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 J121.0546-23.9663 20260121.2703 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:12.90 -23:57:15.6 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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,2461061.7703,14.02,0.05,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 20260121.2703 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:19:24.41 -24:47:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 13.94 08:10:23.04 -24:07:36.1
243.34826 5.04306 galactic Pup Second-epoch detections are separated by 0.7" 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 J122.5960-24.1380 | 08:10:23.05 -24:08:17.0 (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 J122.5960-24.1380,2461061.7703,13.94,0.05,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
ATO J122.5960-24.1380 20260121.2703 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:23.04 -24:07:36.1 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 14.01 08:30:15.65 -28:30:20.5
249.50077 6.27301 galactic Pyx Second-epoch detections are separated by 6.0" 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 5644903112308826752 | 08:30:17.30 -28:30:36.5 (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 5644903112308826752,2461061.7703,14.01,0.05,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 5644903112308826752 20260121.2703 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:15.65 -28:30:20.5 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 14.04 08:25:05.50 -21:38:39.8
243.14444 9.23742 galactic Pup Second-epoch detections are separated by 3.8" 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 J126.2724-21.6449 | 08:25:05.50 -21:38:39.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.298+/-0.116 (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 J126.2724-21.6449,2461061.7703,14.04,0.05,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 J126.2724-21.6449 20260121.2703 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:25:05.50 -21:38:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2703 2461061.7703 14.02 08:06:16.17 -23:19:17.0
242.15883 4.68151 galactic Pup Second-epoch detections are separated by 3.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J121.5660-23.3219 | 08:06:16.17 -23:19:17.0 (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 J121.5660-23.3219,2461061.7703,14.02,0.05,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 J121.5660-23.3219 20260121.2703 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20.00sec_-14.90C_LIGHT_0300.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_003532_TTUQ1b1x1_6866_CQPAOAK6/fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20.00sec_-14.90C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:16.17 -23:19:17.0 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-29-26_20_00sec_-14_90C_LIGHT_0301_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_00-28-39_20_00sec_-14_90C_LIGHT_0300_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.09 19:40:15.06 +57:23:17.7
89.62198 16.42171 galactic Cyg Second-epoch detections are separated by 1.4" 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 | target | 19:40:15.06 +57:23:17.7 (user input) | T | P | (position from user input) J-Ks=0.453+/-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
target,2461061.6116,12.09,0.05,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
target 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:15.06 +57:23:17.7 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.6116,13.95,0.05,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
target 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:49.48 +61:00:05.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.6116,13.08,0.05,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 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:34:36.47 +56:47:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.45 19:45:56.99 +57:22:38.0
89.95539 15.72370 galactic Cyg Second-epoch detections are separated by 0.6" 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 2235239420523452288 | 19:45:56.87 +57:22:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.684+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2235239420523452288,2461061.6116,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2235239420523452288 20260121.1116 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:56.99 +57:22:38.0 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.11 19:45:21.10 +57:00:51.1
89.57963 15.63726 galactic Cyg Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J296.3358+57.0029 | 19:45:20.96 +57:00:51.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.509+/-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 J296.3358+57.0029,2461061.6116,12.11,0.05,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
ATO J296.3358+57.0029 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:21.10 +57:00:51.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.52 19:39:51.96 +57:13:16.2
89.44118 16.39849 galactic Cyg 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 | ATO J294.9646+57.2286 | 19:39:51.89 +57:13:16.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.649+/-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
ATO J294.9646+57.2286,2461061.6116,12.52,0.05,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
ATO J294.9646+57.2286 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:51.96 +57:13:16.2 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 13.23 19:37:37.06 +56:58:29.3
89.07468 16.57288 galactic Cyg Second-epoch detections are separated by 1.6" 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 | target | 19:37:37.06 +56:58:29.3 (user input) | T | P | (position from user input) J-Ks=0.338+/-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,2461061.6116,13.23,0.05,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 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:37:37.06 +56:58:29.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.89 19:38:02.11 +58:25:45.6
90.48311 17.12218 galactic Dra Second-epoch detections are separated by 0.2" 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 | ATO J294.5200+58.4385 | 19:38:02.11 +58:25:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.251+/-0.035 (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 J294.5200+58.4385,2461061.6116,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J294.5200+58.4385 20260121.1116 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:38:02.11 +58:25:45.6 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.57 19:32:57.45 +58:53:56.1
90.65664 17.91522 galactic Dra Second-epoch detections are separated by 0.2" 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 | ATO J293.2387+58.8987 | 19:32:57.29 +58:53:55.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.292+/-0.038 (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 J293.2387+58.8987,2461061.6116,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.2387+58.8987 20260121.1116 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:57.45 +58:53:56.1 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.49 19:39:35.25 +57:19:24.3
89.52142 16.47562 galactic Cyg Second-epoch detections are separated by 1.2" 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 2235281683001041792 | 19:39:30.90 +57:19:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-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 2235281683001041792,2461061.6116,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2235281683001041792 20260121.1116 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:39:35.25 +57:19:24.3 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.15 19:41:37.09 +58:11:24.7
90.46051 16.59479 galactic Cyg Second-epoch detections are separated by 0.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.4038+58.1901 | 19:41:36.92 +58:11:24.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.598+/-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 J295.4038+58.1901,2461061.6116,12.15,0.05,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
ATO J295.4038+58.1901 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:37.09 +58:11:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.76 19:45:36.15 +56:54:40.9
89.49929 15.56139 galactic Cyg Second-epoch detections are separated by 0.5" 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 | ATO J296.3968+56.9109 | 19:45:36.15 +56:54:40.9 (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 J296.3968+56.9109,2461061.6116,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J296.3968+56.9109 20260121.1116 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:45:36.15 +56:54:40.9 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1116 2461061.6116 12.23 19:44:55.14 +57:18:34.0
89.82885 15.81910 galactic Cyg Second-epoch detections are separated by 1.0" 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 | ATO J296.2291+57.3093 | 19:44:54.99 +57:18:33.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.791+/-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 J296.2291+57.3093,2461061.6116,12.23,0.05,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
ATO J296.2291+57.3093 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:55.14 +57:18:34.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.6116,12.98,0.05,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
target 20260121.1116 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-47_20.00sec_-15.00C_LIGHT_0005.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20.00sec_-14.90C_LIGHT_0078.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Cep-05-Q1b1x1_225314_TTUQ1b1x1_11299_6ZTaJans/fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:33:30.67 +56:50:42.3 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-57_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-20_20-40-09_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8133,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3133 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-30-28_20.00sec_-14.90C_LIGHT_0349.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20.00sec_-14.90C_LIGHT_0350.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:49.16 +50:03:53.1 ;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_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_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_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3133 2461061.8133 12.35 08:42:31.99 +53:56:02.3
164.16489 37.78800 galactic UMa Second-epoch detections are separated by 6.2" 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 1030351526051764096 | 08:42:29.55 +53:56:16.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 21.3133* 08 42 31.99 +53 56 02.3 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 1030351526051764096,2461061.8133,12.35,0.05,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 1030351526051764096 20260121.3133 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-30-28_20.00sec_-14.90C_LIGHT_0349.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20.00sec_-14.90C_LIGHT_0350.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:42:31.99 +53:56:02.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_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_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3133 2461061.8133 12.39 08:36:38.23 +53:34:26.3
164.69492 36.94441 galactic UMa Second-epoch detections are separated by 5.8" 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 J129.1784+53.5756 | 08:36:38.23 +53:34:26.3 (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!
TCP 2026 01 21.3133* 08 36 38.23 +53 34 26.3 12.4 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
ATO J129.1784+53.5756,2461061.8133,12.39,0.05,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
ATO J129.1784+53.5756 20260121.3133 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-30-28_20.00sec_-14.90C_LIGHT_0349.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20.00sec_-14.90C_LIGHT_0350.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:36:38.23 +53:34:26.3 ;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_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_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_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3133 2461061.8133 12.38 08:49:43.37 +54:24:14.5
163.43363 38.78728 galactic UMa Second-epoch detections are separated by 7.1" 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 1029976760088920192 | 08:49:42.82 +54:24:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3133* 08 49 43.37 +54 24 14.5 12.4 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 1029976760088920192,2461061.8133,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1029976760088920192 20260121.3133 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-30-28_20.00sec_-14.90C_LIGHT_0349.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20.00sec_-14.90C_LIGHT_0350.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:49:43.37 +54:24:14.5 ;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_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_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_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3133* 08 42 07.55 +54 32 13.1 12.4 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
target,2461061.8133,12.39,0.05,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
target 20260121.3133 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-30-28_20.00sec_-14.90C_LIGHT_0349.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20.00sec_-14.90C_LIGHT_0350.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:42:07.55 +54:32:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_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_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3133* 08 46 10.00 +53 25 40.8 12.1 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
target,2461061.8133,12.05,0.05,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
target 20260121.3133 12.05CV 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-30-28_20.00sec_-14.90C_LIGHT_0349.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_013722_TTUQ1b1x1_4077_YVnVITZ2/fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20.00sec_-14.90C_LIGHT_0350.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:46:10.00 +53:25:40.8 ;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_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_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_2026-01-21_01-31-24_20_00sec_-14_90C_LIGHT_0350_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_2026-01-21_01-30-28_20_00sec_-14_90C_LIGHT_0349_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7837,14.25,0.05,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
target 20260121.2837 14.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Mon-06-Q1b1x1_015926_TTUQ1b1x1_6778_hoXAoA0Q/fd_Mon-06-Q1b1x1_2026-01-21_00-47-51_20.00sec_-15.00C_LIGHT_0310.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_015926_TTUQ1b1x1_6778_hoXAoA0Q/fd_Mon-06-Q1b1x1_2026-01-21_00-48-44_20.00sec_-14.90C_LIGHT_0311.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:14.60 -14:07:52.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-21_00-48-44_20_00sec_-14_90C_LIGHT_0311_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_2026-01-21_00-47-51_20_00sec_-15_00C_LIGHT_0310_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_2026-01-21_00-48-44_20_00sec_-14_90C_LIGHT_0311_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_2026-01-21_00-47-51_20_00sec_-15_00C_LIGHT_0310_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2837 2461061.7837 13.05 07:11:53.14 -14:23:36.5
228.04712 -2.09393 galactic CMa 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 | target | 07:11:53.14 -14:23:36.5 (user input) | T | P | (position from user input) J-Ks=0.372+/-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
target,2461061.7837,13.05,0.05,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
target 20260121.2837 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-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-40-07_20.00sec_-15.00C_LIGHT_0391.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_015926_TTUQ1b1x1_6778_hoXAoA0Q/fd_Mon-06-Q1b1x1_2026-01-21_00-47-51_20.00sec_-15.00C_LIGHT_0310.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_015926_TTUQ1b1x1_6778_hoXAoA0Q/fd_Mon-06-Q1b1x1_2026-01-21_00-48-44_20.00sec_-14.90C_LIGHT_0311.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:53.14 -14:23:36.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-21_00-48-44_20_00sec_-14_90C_LIGHT_0311_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_2026-01-21_00-47-51_20_00sec_-15_00C_LIGHT_0310_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_2026-01-21_00-48-44_20_00sec_-14_90C_LIGHT_0311_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_2026-01-21_00-47-51_20_00sec_-15_00C_LIGHT_0310_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3559* 03 11 39.62 +57 53 50.3 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8559,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3559 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-08-Q1b1x1_2025-12-23_00-44-54_20.00sec_-14.90C_LIGHT_0330.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-08-Q1b1x1_025245_TTUQ1b1x1_32656_0fIICwOo/fd_Cam-08-Q1b1x1_2026-01-21_02-31-50_20.00sec_-15.00C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-08-Q1b1x1_025245_TTUQ1b1x1_32656_0fIICwOo/fd_Cam-08-Q1b1x1_2026-01-21_02-32-51_20.00sec_-15.00C_LIGHT_0400.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:11:39.62 +57:53:50.3 ;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_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-01-21_02-32-51_20_00sec_-15_00C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-01-21_02-31-50_20_00sec_-15_00C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-01-21_02-32-51_20_00sec_-15_00C_LIGHT_0400_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-01-21_02-31-50_20_00sec_-15_00C_LIGHT_0399_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3559 2461061.8559 14.11 03:57:32.58 +61:31:30.1
143.30061 6.25060 galactic Cam Second-epoch detections are separated by 0.3" 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 474683736923834880 | 03:57:37.85 +61:31:34.9 (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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 474683736923834880,2461061.8559,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 474683736923834880 20260121.3559 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cam-08-Q1b1x1_2025-12-23_00-44-54_20.00sec_-14.90C_LIGHT_0330.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-08-Q1b1x1_025245_TTUQ1b1x1_32656_0fIICwOo/fd_Cam-08-Q1b1x1_2026-01-21_02-31-50_20.00sec_-15.00C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-08-Q1b1x1_025245_TTUQ1b1x1_32656_0fIICwOo/fd_Cam-08-Q1b1x1_2026-01-21_02-32-51_20.00sec_-15.00C_LIGHT_0400.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:32.58 +61:31:30.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-01-21_02-32-51_20_00sec_-15_00C_LIGHT_0400_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-01-21_02-31-50_20_00sec_-15_00C_LIGHT_0399_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-01-21_02-32-51_20_00sec_-15_00C_LIGHT_0400_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-08-Q1b1x1_2025-12-23_00-44-54_20_00sec_-14_90C_LIGHT_0330_fits__*pix.png resample_wcs_fd_Cam-08-Q1b1x1_2026-01-21_02-31-50_20_00sec_-15_00C_LIGHT_0399_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3601 2461061.8601 14.11 05:32:35.78 +34:52:06.7
173.50855 0.82568 galactic Aur Second-epoch detections are separated by 2.0" and 2.2 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 J083.1561+34.8462 | 05:32:36.50 +34:51:25.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.1561+34.8462,2461061.8601,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.1561+34.8462 20260121.3601 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2025-12-23_01-48-53_20.00sec_-15.00C_LIGHT_0395.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-03-Q1b1x1_025643_TTUQ1b1x1_20650_nTDpGRHG/fd_Aur-03-Q1b1x1_2026-01-21_02-38-01_20.00sec_-15.00C_LIGHT_0404.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-03-Q1b1x1_025643_TTUQ1b1x1_20650_nTDpGRHG/fd_Aur-03-Q1b1x1_2026-01-21_02-38-39_20.00sec_-14.90C_LIGHT_0405.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:35.78 +34:52:06.7 ;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_Aur-03-Q1b1x1_2025-12-23_01-48-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Aur-03-Q1b1x1_2026-01-21_02-38-39_20_00sec_-14_90C_LIGHT_0405_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q1b1x1_2025-12-23_01-48-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Aur-03-Q1b1x1_2026-01-21_02-38-01_20_00sec_-15_00C_LIGHT_0404_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q1b1x1_2025-12-23_01-48-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Aur-03-Q1b1x1_2026-01-21_02-38-39_20_00sec_-14_90C_LIGHT_0405_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q1b1x1_2025-12-23_01-48-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Aur-03-Q1b1x1_2026-01-21_02-38-01_20_00sec_-15_00C_LIGHT_0404_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3601 2461061.8601 14.24 05:45:33.26 +42:05:40.1
168.70912 6.80132 galactic Aur Second-epoch detections are separated by 5.4" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J086.3868+42.1174 | 05:45:32.07 +42:06:20.8 (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 J086.3868+42.1174,2461061.8601,14.24,0.05,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 J086.3868+42.1174 20260121.3601 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2025-12-23_01-48-53_20.00sec_-15.00C_LIGHT_0395.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-03-Q1b1x1_025643_TTUQ1b1x1_20650_nTDpGRHG/fd_Aur-03-Q1b1x1_2026-01-21_02-38-01_20.00sec_-15.00C_LIGHT_0404.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-03-Q1b1x1_025643_TTUQ1b1x1_20650_nTDpGRHG/fd_Aur-03-Q1b1x1_2026-01-21_02-38-39_20.00sec_-14.90C_LIGHT_0405.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:33.26 +42:05:40.1 ;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_Aur-03-Q1b1x1_2025-12-23_01-48-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Aur-03-Q1b1x1_2026-01-21_02-38-39_20_00sec_-14_90C_LIGHT_0405_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q1b1x1_2025-12-23_01-48-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Aur-03-Q1b1x1_2026-01-21_02-38-01_20_00sec_-15_00C_LIGHT_0404_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q1b1x1_2025-12-23_01-48-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Aur-03-Q1b1x1_2026-01-21_02-38-39_20_00sec_-14_90C_LIGHT_0405_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q1b1x1_2025-12-23_01-48-53_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Aur-03-Q1b1x1_2026-01-21_02-38-01_20_00sec_-15_00C_LIGHT_0404_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8027,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3027 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-15-19_20.00sec_-15.00C_LIGHT_0339.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20.00sec_-14.90C_LIGHT_0340.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:49.94 +00:48:05.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_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_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3027 2461061.8027 13.56 07:11:37.80 +06:38:48.0
209.27939 7.50211 galactic CMi Second-epoch detections are separated by 0.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.9077+06.6454 | 07:11:36.68 +06:39:13.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9077+06.6454,2461061.8027,13.56,0.05,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
ATO J107.9077+06.6454 20260121.3027 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/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-15-19_20.00sec_-15.00C_LIGHT_0339.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20.00sec_-14.90C_LIGHT_0340.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:37.80 +06:38:48.0 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_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_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3027 2461061.8027 14.39 07:12:20.29 +07:10:52.2
208.87624 7.89829 galactic CMi 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 3153413337174780544 | 07:12:21.30 +07:11:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3153413337174780544,2461061.8027,14.39,0.05,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
Gaia DR3 3153413337174780544 20260121.3027 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/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-15-19_20.00sec_-15.00C_LIGHT_0339.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20.00sec_-14.90C_LIGHT_0340.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:20.29 +07:10:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_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_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8027,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3027 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/CMi-01-Q1b1x1_2025-12-23_02-47-07_20.00sec_-14.90C_LIGHT_0449.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-15-19_20.00sec_-15.00C_LIGHT_0339.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20.00sec_-14.90C_LIGHT_0340.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:25:44.55 +09:46:41.2 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_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_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3027 2461061.8027 14.49 07:17:26.24 +02:32:00.2
213.63774 6.93850 galactic CMi Second-epoch detections are separated by 5.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.3554+02.5339 | 07:17:26.24 +02:32:00.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.3554+02.5339,2461061.8027,14.49,0.05,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 J109.3554+02.5339 20260121.3027 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_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-15-19_20.00sec_-15.00C_LIGHT_0339.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_015742_TTUQ1b1x1_14378_kd3cmg9c/fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20.00sec_-14.90C_LIGHT_0340.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:17:26.24 +02:32:00.2 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_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_2026-01-21_01-16-08_20_00sec_-14_90C_LIGHT_0340_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_2026-01-21_01-15-19_20_00sec_-15_00C_LIGHT_0339_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3382 2461061.8382 13.92 04:10:49.28 +42:10:39.4
157.71492 -6.84251 galactic Per Second-epoch detections are separated by 3.3" 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 | ATO J062.7182+42.1810 | 04:10:49.28 +42:10:39.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3382* 04 10 49.28 +42 10 39.4 13.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J062.7182+42.1810,2461061.8382,13.92,0.05,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
ATO J062.7182+42.1810 20260121.3382 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-05-Q1b1x1_022759_TTUQ1b1x1_12148_FdgN9VmZ/fd_Per-05-Q1b1x1_2026-01-21_02-06-23_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-05-Q1b1x1_022759_TTUQ1b1x1_12148_FdgN9VmZ/fd_Per-05-Q1b1x1_2026-01-21_02-07-23_20.00sec_-14.90C_LIGHT_0375.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:49.28 +42:10:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-01-21_02-07-23_20_00sec_-14_90C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-01-21_02-06-23_20_00sec_-14_90C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-01-21_02-07-23_20_00sec_-14_90C_LIGHT_0375_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-01-21_02-06-23_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3382 2461061.8382 14.22 04:29:15.15 +39:20:33.3
162.21602 -6.37708 galactic Per Second-epoch detections are separated by 1.5" 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 | ATO J067.3122+39.3394 | 04:29:13.59 +39:21:05.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.535+/-0.040 (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 21.3382* 04 29 15.15 +39 20 33.3 14.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J067.3122+39.3394,2461061.8382,14.22,0.05,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
ATO J067.3122+39.3394 20260121.3382 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/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-05-Q1b1x1_022759_TTUQ1b1x1_12148_FdgN9VmZ/fd_Per-05-Q1b1x1_2026-01-21_02-06-23_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-05-Q1b1x1_022759_TTUQ1b1x1_12148_FdgN9VmZ/fd_Per-05-Q1b1x1_2026-01-21_02-07-23_20.00sec_-14.90C_LIGHT_0375.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:15.15 +39:20:33.3 ;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_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-01-21_02-07-23_20_00sec_-14_90C_LIGHT_0375_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-01-21_02-06-23_20_00sec_-14_90C_LIGHT_0374_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-01-21_02-07-23_20_00sec_-14_90C_LIGHT_0375_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-01-21_02-06-23_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3718 2461061.8718 13.65 10:07:01.70 -27:16:09.4
263.60249 22.77951 galactic Ant Second-epoch detections are separated by 1.3" and 10.1 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 5466432510885908480 | 10:07:02.58 -27:15:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3718* 10 07 01.70 -27 16 09.4 13.7 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 5466432510885908480,2461061.8718,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5466432510885908480 20260121.3718 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:07:01.70 -27:16:09.4 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_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_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3718* 10 10 14.08 -27 58 47.0 14.1 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
target,2461061.8718,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3718 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/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:10:14.08 -27:58:47.0 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_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_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8718,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3718 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:05.17 -27:05:01.6 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_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_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3718* 10 09 30.59 -27 28 52.0 14.2 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
target,2461061.8718,14.21,0.05,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
target 20260121.3718 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/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:30.59 -27:28:52.0 ;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-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_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_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3718* 10 09 59.39 -27 48 58.3 14.3 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
target,2461061.8718,14.26,0.05,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 20260121.3718 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/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_031446_TTUQ1b1x1_8633_wImuZGqo/fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20.00sec_-15.00C_LIGHT_0423.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:59.39 -27:48:58.3 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_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_2026-01-21_02-55-45_20_00sec_-15_00C_LIGHT_0423_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_2026-01-21_02-54-45_20_00sec_-14_90C_LIGHT_0422_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1829 2461061.6829 11.96 04:50:45.23 -22:24:52.5
221.99618 -35.97049 galactic Eri Second-epoch detections are separated by 0.5" 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 | Gaia DR3 2973653390873446784 | 04:50:45.17 -22:24:52.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.262+/-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 21.1829* 04 50 45.23 -22 24 52.5 12.0 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 2973653390873446784,2461061.6829,11.96,0.05,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 2973653390873446784 20260121.1829 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/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_2026-01-21_CI_Lep-01-Q1b1x1_002526_TTUQ1b1x1_31067_MZ2L0ziD/fd_Lep-01-Q1b1x1_2026-01-20_22-22-49_20.00sec_-14.90C_LIGHT_0180.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lep-01-Q1b1x1_002526_TTUQ1b1x1_31067_MZ2L0ziD/fd_Lep-01-Q1b1x1_2026-01-20_22-23-37_20.00sec_-14.90C_LIGHT_0181.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:45.23 -22:24:52.5 ;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_Lep-01-Q1b1x1_2025-12-22_23-23-57_20_00sec_-15_00C_LIGHT_0236_fits__*pix.png resample_wcs_fd_Lep-01-Q1b1x1_2026-01-20_22-23-37_20_00sec_-14_90C_LIGHT_0181_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_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_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_2026-01-20_22-23-37_20_00sec_-14_90C_LIGHT_0181_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_2026-01-20_22-22-49_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3663 2461061.8663 12.87 01:06:15.00 +65:44:33.1
124.45435 2.91457 galactic Cas Second-epoch detections are separated by 0.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:15.00 +65:44:33.1 (user input) | T | P | (position from user input) J-Ks=0.379+/-0.029 (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 21.3663* 01 06 15.00 +65 44 33.1 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8663,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3663 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cas-01-Q1b1x1_2025-12-23_00-01-41_20.00sec_-15.00C_LIGHT_0280.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cas-01-Q1b1x1_2025-12-23_00-02-35_20.00sec_-15.00C_LIGHT_0281.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cas-01-Q1b1x1_025046_TTUQ1b1x1_32065_4GozlICu/fd_Cas-01-Q1b1x1_2026-01-21_02-46-42_20.00sec_-14.90C_LIGHT_0413.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cas-01-Q1b1x1_025046_TTUQ1b1x1_32065_4GozlICu/fd_Cas-01-Q1b1x1_2026-01-21_02-47-46_20.00sec_-14.90C_LIGHT_0414.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:06:15.00 +65:44:33.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cas-01-Q1b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q1b1x1_2026-01-21_02-47-46_20_00sec_-14_90C_LIGHT_0414_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-01-Q1b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q1b1x1_2026-01-21_02-46-42_20_00sec_-14_90C_LIGHT_0413_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cas-01-Q1b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q1b1x1_2026-01-21_02-47-46_20_00sec_-14_90C_LIGHT_0414_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-01-Q1b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q1b1x1_2026-01-21_02-46-42_20_00sec_-14_90C_LIGHT_0413_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3681 2461061.8681 11.11 05:34:19.96 -05:27:12.4
208.95859 -19.62193 galactic Ori Second-epoch detections are separated by 2.0" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3209422386474525824 | 05:34:19.49 -05:27:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5IV/V 1975MNRAS.171..219P Parenago 1423
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3681* 05 34 19.96 -05 27 12.4 11.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3209422386474525824,2461061.8681,11.11,0.05,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 3209422386474525824 20260121.3681 11.11CV 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/Ori-06-Q1b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-49-37_20.00sec_-15.00C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:19.96 -05:27:12.4 ;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_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_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_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3681 2461061.8681 12.61 05:29:11.68 -07:13:44.2
210.04274 -21.55899 galactic Ori Second-epoch detections are separated by 0.4" and 2.2 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 3016601341549787904 | 05:29:11.35 -07:13:47.6 (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 21.3681* 05 29 11.68 -07 13 44.2 12.6 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 3016601341549787904,2461061.8681,12.61,0.05,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
Gaia DR3 3016601341549787904 20260121.3681 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/Ori-06-Q1b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-49-37_20.00sec_-15.00C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:11.68 -07:13:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_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_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3681 2461061.8681 12.79 05:28:50.73 -07:08:40.9
209.92019 -21.59914 galactic Ori Second-epoch detections are separated by 0.8" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:28:50.73 -07:08:40.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3681* 05 28 50.73 -07 08 40.9 12.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8681,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3681 12.79CV 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/Ori-06-Q1b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-49-37_20.00sec_-15.00C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:50.73 -07:08:40.9 ;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_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_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_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3681 2461061.8681 13.09 05:28:45.98 -07:13:07.0
209.98203 -21.64958 galactic Ori Second-epoch detections are separated by 2.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:28:45.98 -07:13:07.0 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3681* 05 28 45.98 -07 13 07.0 13.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8681,13.09,0.05,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
target 20260121.3681 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-49-37_20.00sec_-15.00C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:45.98 -07:13:07.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_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_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3681 2461061.8681 13.57 05:28:58.16 -07:14:51.8
210.03414 -21.61740 galactic Ori Second-epoch detections are separated by 2.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:28:58.16 -07:14:51.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3681* 05 28 58.16 -07 14 51.8 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8681,13.57,0.05,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 20260121.3681 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/Ori-06-Q1b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-49-37_20.00sec_-15.00C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:58.16 -07:14:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_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_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3681 2461061.8681 14.14 05:41:44.66 -01:45:12.8
206.39751 -16.27919 galactic Ori Second-epoch detections are separated by 5.6" 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 | ATO J085.4369-01.7579 | 05:41:44.66 -01:45:12.8 (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 21.3681* 05 41 44.66 -01 45 12.8 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.4369-01.7579,2461061.8681,14.14,0.05,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
ATO J085.4369-01.7579 20260121.3681 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/Ori-06-Q1b1x1_2025-12-23_00-51-32_20.00sec_-15.00C_LIGHT_0338.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-49-37_20.00sec_-15.00C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_030647_TTUQ1b1x1_5856_cpH4MujB/fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20.00sec_-15.00C_LIGHT_0417.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:44.66 -01:45:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_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_2026-01-21_02-50-13_20_00sec_-15_00C_LIGHT_0417_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_2026-01-21_02-49-37_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3843 2461061.8843 14.07 08:03:25.97 +10:03:06.3
211.91627 20.50981 galactic Cnc Second-epoch detections are separated by 4.0" 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 J120.8563+10.0506 | 08:03:25.97 +10:03:06.3 (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 J120.8563+10.0506,2461061.8843,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J120.8563+10.0506 20260121.3843 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_CMi-01-Q1b1x1_033243_TTUQ1b1x1_7941_xT5IDM3e/fd_CMi-01-Q1b1x1_2026-01-21_03-12-48_20.00sec_-14.90C_LIGHT_0439.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_033243_TTUQ1b1x1_7941_xT5IDM3e/fd_CMi-01-Q1b1x1_2026-01-21_03-13-36_20.00sec_-15.00C_LIGHT_0440.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:25.97 +10:03:06.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-21_03-13-36_20_00sec_-15_00C_LIGHT_0440_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_2026-01-21_03-12-48_20_00sec_-14_90C_LIGHT_0439_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_2026-01-21_03-13-36_20_00sec_-15_00C_LIGHT_0440_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_2026-01-21_03-12-48_20_00sec_-14_90C_LIGHT_0439_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3843 2461061.8843 13.94 07:20:29.65 +06:15:40.9
210.62323 9.29933 galactic CMi Second-epoch detections are separated by 2.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J110.1323+06.2532 | 07:20:29.65 +06:15:40.9 (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 J110.1323+06.2532,2461061.8843,13.94,0.05,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
ATO J110.1323+06.2532 20260121.3843 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_CMi-01-Q1b1x1_033243_TTUQ1b1x1_7941_xT5IDM3e/fd_CMi-01-Q1b1x1_2026-01-21_03-12-48_20.00sec_-14.90C_LIGHT_0439.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMi-01-Q1b1x1_033243_TTUQ1b1x1_7941_xT5IDM3e/fd_CMi-01-Q1b1x1_2026-01-21_03-13-36_20.00sec_-15.00C_LIGHT_0440.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:20:29.65 +06:15:40.9 ;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_CMi-01-Q1b1x1_2025-12-23_02-47-07_20_00sec_-14_90C_LIGHT_0449_fits__*pix.png resample_wcs_fd_CMi-01-Q1b1x1_2026-01-21_03-13-36_20_00sec_-15_00C_LIGHT_0440_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_2026-01-21_03-12-48_20_00sec_-14_90C_LIGHT_0439_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_2026-01-21_03-13-36_20_00sec_-15_00C_LIGHT_0440_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_2026-01-21_03-12-48_20_00sec_-14_90C_LIGHT_0439_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.4082* 10 38 50.35 -11 38 49.5 14.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.9082,14.42,0.05,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
target 20260121.4082 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/Sex-03-Q1b1x1_2025-12-23_03-51-09_20.00sec_-14.90C_LIGHT_0518.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Sex-03-Q1b1x1_035246_TTUQ1b1x1_22169_EL0eMo8D/fd_Sex-03-Q1b1x1_2026-01-21_03-47-10_20.00sec_-14.90C_LIGHT_0474.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Sex-03-Q1b1x1_035246_TTUQ1b1x1_22169_EL0eMo8D/fd_Sex-03-Q1b1x1_2026-01-21_03-48-14_20.00sec_-14.90C_LIGHT_0475.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:38:50.35 -11:38:49.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-03-Q1b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q1b1x1_2026-01-21_03-48-14_20_00sec_-14_90C_LIGHT_0475_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-03-Q1b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q1b1x1_2026-01-21_03-47-10_20_00sec_-14_90C_LIGHT_0474_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-03-Q1b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q1b1x1_2026-01-21_03-48-14_20_00sec_-14_90C_LIGHT_0475_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-03-Q1b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q1b1x1_2026-01-21_03-47-10_20_00sec_-14_90C_LIGHT_0474_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4070 2461061.9070 12.46 11:09:34.74 -13:10:21.3
268.19068 42.72433 galactic Crt Second-epoch detections are separated by 0.2" 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 | ATO J167.3948-13.1725 | 11:09:34.75 -13:10:21.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.373+/-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 J167.3948-13.1725,2461061.9070,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J167.3948-13.1725 20260121.4070 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-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_2026-01-21_CI_Hya-09-Q1b1x1_035500_TTUQ1b1x1_31710_xz9OXihy/fd_Hya-09-Q1b1x1_2026-01-21_03-45-24_20.00sec_-15.00C_LIGHT_0472.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-09-Q1b1x1_035500_TTUQ1b1x1_31710_xz9OXihy/fd_Hya-09-Q1b1x1_2026-01-21_03-46-24_20.00sec_-15.00C_LIGHT_0473.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:09:34.74 -13:10:21.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-01-21_03-46-24_20_00sec_-15_00C_LIGHT_0473_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_2026-01-21_03-45-24_20_00sec_-15_00C_LIGHT_0472_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_2026-01-21_03-46-24_20_00sec_-15_00C_LIGHT_0473_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_2026-01-21_03-45-24_20_00sec_-15_00C_LIGHT_0472_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2177 2461061.7177 10.21 10:12:08.52 -30:54:28.1
266.97935 20.62444 galactic Ant Second-epoch detections are separated by 1.0" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 21.2177* 10 12 08.52 -30 54 28.1 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 5461813157597324288,2461061.7177,10.21,0.05,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
Gaia DR3 5461813157597324288 20260121.2177 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/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_003738_TTUQ1b1x1_7419_AVLjqYq1/fd_Ant-01-Q1b1x1_2026-01-20_23-12-57_20.00sec_-15.00C_LIGHT_0230.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_003738_TTUQ1b1x1_7419_AVLjqYq1/fd_Ant-01-Q1b1x1_2026-01-20_23-13-35_20.00sec_-15.00C_LIGHT_0231.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:12:08.52 -30:54:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-20_23-13-35_20_00sec_-15_00C_LIGHT_0231_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_2026-01-20_23-12-57_20_00sec_-15_00C_LIGHT_0230_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_2026-01-20_23-13-35_20_00sec_-15_00C_LIGHT_0231_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_2026-01-20_23-12-57_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2177 2461061.7177 11.18 10:10:57.40 -30:58:45.9
266.81109 20.41257 galactic Ant Second-epoch detections are separated by 1.1" 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 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 21.2177* 10 10 57.40 -30 58 45.9 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 5460313767336112128,2461061.7177,11.18,0.05,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 5460313767336112128 20260121.2177 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-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_003738_TTUQ1b1x1_7419_AVLjqYq1/fd_Ant-01-Q1b1x1_2026-01-20_23-12-57_20.00sec_-15.00C_LIGHT_0230.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_003738_TTUQ1b1x1_7419_AVLjqYq1/fd_Ant-01-Q1b1x1_2026-01-20_23-13-35_20.00sec_-15.00C_LIGHT_0231.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:10:57.40 -30:58:45.9 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-20_23-13-35_20_00sec_-15_00C_LIGHT_0231_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_2026-01-20_23-12-57_20_00sec_-15_00C_LIGHT_0230_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_2026-01-20_23-13-35_20_00sec_-15_00C_LIGHT_0231_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_2026-01-20_23-12-57_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2177 2461061.7177 11.34 10:01:08.51 -30:23:07.3
264.66393 19.55584 galactic Ant Second-epoch detections are separated by 1.2" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | NSV 4706 | 10:01:09.38 -30:23:14.2 (Gaia DR3) | CST (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: M3V 1983SAAOC...7..106W LHS 277
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 21.2177* 10 01 08.51 -30 23 07.3 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
NSV 4706,2461061.7177,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 4706 20260121.2177 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Ant-01-Q1b1x1_003738_TTUQ1b1x1_7419_AVLjqYq1/fd_Ant-01-Q1b1x1_2026-01-20_23-12-57_20.00sec_-15.00C_LIGHT_0230.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_003738_TTUQ1b1x1_7419_AVLjqYq1/fd_Ant-01-Q1b1x1_2026-01-20_23-13-35_20.00sec_-15.00C_LIGHT_0231.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:01:08.51 -30:23:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-20_23-13-35_20_00sec_-15_00C_LIGHT_0231_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_2026-01-20_23-12-57_20_00sec_-15_00C_LIGHT_0230_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_2026-01-20_23-13-35_20_00sec_-15_00C_LIGHT_0231_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_2026-01-20_23-12-57_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2177 2461061.7177 11.45 10:11:01.65 -30:57:33.8
266.81083 20.43770 galactic Ant Second-epoch detections are separated by 1.7" 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 5460313801695229696 | 10:11:02.51 -30:57:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 21.2177* 10 11 01.65 -30 57 33.8 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 5460313801695229696,2461061.7177,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5460313801695229696 20260121.2177 11.45CV 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/Ant-01-Q1b1x1_2026-01-09_02-35-22_20.00sec_-15.00C_LIGHT_0012.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_003738_TTUQ1b1x1_7419_AVLjqYq1/fd_Ant-01-Q1b1x1_2026-01-20_23-12-57_20.00sec_-15.00C_LIGHT_0230.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ant-01-Q1b1x1_003738_TTUQ1b1x1_7419_AVLjqYq1/fd_Ant-01-Q1b1x1_2026-01-20_23-13-35_20.00sec_-15.00C_LIGHT_0231.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:11:01.65 -30:57:33.8 ;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_Ant-01-Q1b1x1_2026-01-09_02-35-22_20_00sec_-15_00C_LIGHT_0012_fits__*pix.png resample_wcs_fd_Ant-01-Q1b1x1_2026-01-20_23-13-35_20_00sec_-15_00C_LIGHT_0231_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_2026-01-20_23-12-57_20_00sec_-15_00C_LIGHT_0230_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_2026-01-20_23-13-35_20_00sec_-15_00C_LIGHT_0231_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_2026-01-20_23-12-57_20_00sec_-15_00C_LIGHT_0230_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3791 2461061.8791 14.40 07:45:33.11 -05:30:30.5
224.13108 9.40784 galactic Mon Second-epoch detections are separated by 8.7" 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 3056329346661297920 | 07:45:32.68 -05:30:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3056329346661297920,2461061.8791,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3056329346661297920 20260121.3791 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2025-12-23_02-26-39_20.00sec_-15.00C_LIGHT_0429.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-03-Q1b1x1_030907_TTUQ1b1x1_16481_CISeY9Ej/fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20.00sec_-15.00C_LIGHT_0432.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-03-Q1b1x1_030907_TTUQ1b1x1_16481_CISeY9Ej/fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20.00sec_-14.90C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:33.11 -05:30:30.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20_00sec_-14_90C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20_00sec_-14_90C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8791,13.71,0.05,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 20260121.3791 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/Mon-03-Q1b1x1_2025-12-23_02-26-39_20.00sec_-15.00C_LIGHT_0429.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-03-Q1b1x1_030907_TTUQ1b1x1_16481_CISeY9Ej/fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20.00sec_-15.00C_LIGHT_0432.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-03-Q1b1x1_030907_TTUQ1b1x1_16481_CISeY9Ej/fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20.00sec_-14.90C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:42.69 -00:16:45.1 ;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_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20_00sec_-14_90C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20_00sec_-14_90C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3791 2461061.8791 13.88 07:11:55.81 +00:47:38.2
214.56427 4.92101 galactic Mon Second-epoch detections are separated by 5.0" 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 | ASAS J071154+0047.6 | 07:11:53.37 +00:47:36.3 (Gaia DR3) | SR (local) | 2458232.37680 (local) | Gaia3var=VARIABLE SpType: M6 1993yCat.3170....0M IRAS 07093+0052
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J071154+0047.6,2461061.8791,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J071154+0047.6 20260121.3791 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2025-12-23_02-26-39_20.00sec_-15.00C_LIGHT_0429.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-03-Q1b1x1_030907_TTUQ1b1x1_16481_CISeY9Ej/fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20.00sec_-15.00C_LIGHT_0432.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-03-Q1b1x1_030907_TTUQ1b1x1_16481_CISeY9Ej/fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20.00sec_-14.90C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:55.81 +00:47:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20_00sec_-14_90C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20_00sec_-14_90C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3791 2461061.8791 14.16 07:14:31.02 -01:41:34.5
217.07930 4.35648 galactic Mon Second-epoch detections are separated by 3.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.6276-01.6833 | 07:14:31.02 -01:41:34.5 (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 J108.6276-01.6833,2461061.8791,14.16,0.05,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 J108.6276-01.6833 20260121.3791 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-03-Q1b1x1_2025-12-23_02-26-39_20.00sec_-15.00C_LIGHT_0429.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-03-Q1b1x1_030907_TTUQ1b1x1_16481_CISeY9Ej/fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20.00sec_-15.00C_LIGHT_0432.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-03-Q1b1x1_030907_TTUQ1b1x1_16481_CISeY9Ej/fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20.00sec_-14.90C_LIGHT_0433.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:31.02 -01:41:34.5 ;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_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20_00sec_-14_90C_LIGHT_0433_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20_00sec_-15_00C_LIGHT_0432_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-06-12_20_00sec_-14_90C_LIGHT_0433_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-03-Q1b1x1_2025-12-23_02-26-39_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png resample_wcs_fd_Mon-03-Q1b1x1_2026-01-21_03-05-23_20_00sec_-15_00C_LIGHT_0432_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.1893* 02 27 07.40 +48 08 35.3 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.6892,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.1892 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-20_CI_And-03-Q1b1x1_225923_TTUQ1b1x1_14056_QH9saBHu/fd_And-03-Q1b1x1_2026-01-20_22-31-45_20.00sec_-15.00C_LIGHT_0190.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_And-03-Q1b1x1_225923_TTUQ1b1x1_14056_QH9saBHu/fd_And-03-Q1b1x1_2026-01-20_22-32-57_20.00sec_-14.90C_LIGHT_0191.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:27:07.40 +48:08:35.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-01-20_22-32-57_20_00sec_-14_90C_LIGHT_0191_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_2026-01-20_22-31-45_20_00sec_-15_00C_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_And-03-Q1b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_fd_And-03-Q1b1x1_2026-01-20_22-32-57_20_00sec_-14_90C_LIGHT_0191_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_2026-01-20_22-31-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2204 2461061.7204 14.38 06:37:58.51 +34:29:45.5
180.33492 12.42627 galactic Aur Second-epoch detections are separated by 2.1" 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 941462504937668864 | 06:37:55.44 +34:29:24.7 (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 941462504937668864,2461061.7204,14.38,0.05,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 941462504937668864 20260121.2204 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-01-Q1b1x1_2025-12-23_02-54-13_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-01-Q1b1x1_232209_TTUQ1b1x1_27973_z6N3UjMh/fd_Gem-01-Q1b1x1_2026-01-20_23-16-36_20.00sec_-15.00C_LIGHT_0234.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-20_CI_Gem-01-Q1b1x1_232209_TTUQ1b1x1_27973_z6N3UjMh/fd_Gem-01-Q1b1x1_2026-01-20_23-17-45_20.00sec_-14.90C_LIGHT_0235.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:58.51 +34:29:45.5 ;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_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-17-45_20_00sec_-14_90C_LIGHT_0235_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-16-36_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-17-45_20_00sec_-14_90C_LIGHT_0235_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-16-36_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.1865 2461061.6865 14.45 04:30:50.98 -05:47:53.6
201.04439 -33.76518 galactic Eri Second-epoch detections are separated by 1.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J067.7150-05.7981 | 04:30:50.98 -05:47:53.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.1865* 04 30 50.98 -05 47 53.6 14.4 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
ATO J067.7150-05.7981,2461061.6865,14.45,0.05,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 J067.7150-05.7981 20260121.1865 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/Eri-02-Q1b1x1_2025-12-22_23-45-40_20.00sec_-14.90C_LIGHT_0260.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Eri-02-Q1b1x1_000318_TTUQ1b1x1_19972_cb3YXO7R/fd_Eri-02-Q1b1x1_2026-01-20_22-27-59_20.00sec_-14.90C_LIGHT_0186.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Eri-02-Q1b1x1_000318_TTUQ1b1x1_19972_cb3YXO7R/fd_Eri-02-Q1b1x1_2026-01-20_22-28-55_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:30:50.98 -05:47:53.6 ;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_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-01-20_22-28-55_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-01-20_22-27-59_20_00sec_-14_90C_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_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-01-20_22-28-55_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-02-Q1b1x1_2025-12-22_23-45-40_20_00sec_-14_90C_LIGHT_0260_fits__*pix.png resample_wcs_fd_Eri-02-Q1b1x1_2026-01-20_22-27-59_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.9287,14.32,0.05,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 20260121.4287 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/Cam-01-Q1b1x1_2025-12-23_02-44-02_20.00sec_-15.00C_LIGHT_0445.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-01-Q1b1x1_041843_TTUQ1b1x1_3457_JQvpHqPY/fd_Cam-01-Q1b1x1_2026-01-21_04-16-48_20.00sec_-15.00C_LIGHT_0496.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-01-Q1b1x1_041843_TTUQ1b1x1_3457_JQvpHqPY/fd_Cam-01-Q1b1x1_2026-01-21_04-17-39_20.00sec_-15.00C_LIGHT_0497.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:27.78 +85:18:22.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-01-21_04-17-39_20_00sec_-15_00C_LIGHT_0497_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-01-21_04-16-48_20_00sec_-15_00C_LIGHT_0496_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-01-21_04-17-39_20_00sec_-15_00C_LIGHT_0497_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-01-Q1b1x1_2025-12-23_02-44-02_20_00sec_-15_00C_LIGHT_0445_fits__*pix.png resample_wcs_fd_Cam-01-Q1b1x1_2026-01-21_04-16-48_20_00sec_-15_00C_LIGHT_0496_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3646 2461061.8646 14.38 07:14:11.00 +18:56:43.3
198.27157 13.38234 galactic Gem Second-epoch detections are separated by 4.2" 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 J108.5458+18.9450 | 07:14:11.00 +18:56:43.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.996+/-0.098 (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 J108.5458+18.9450,2461061.8646,14.38,0.05,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 J108.5458+18.9450 20260121.3646 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_2026-01-21_CI_Gem-05-Q1b1x1_030518_TTUQ1b1x1_14931_hqH9ahqi/fd_Gem-05-Q1b1x1_2026-01-21_02-44-06_20.00sec_-15.00C_LIGHT_0411.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-05-Q1b1x1_030518_TTUQ1b1x1_14931_hqH9ahqi/fd_Gem-05-Q1b1x1_2026-01-21_02-45-27_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:11.00 +18:56:43.3 ;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_2026-01-21_02-45-27_20_00sec_-15_00C_LIGHT_0412_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_2026-01-21_02-44-06_20_00sec_-15_00C_LIGHT_0411_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_2026-01-21_02-45-27_20_00sec_-15_00C_LIGHT_0412_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_2026-01-21_02-44-06_20_00sec_-15_00C_LIGHT_0411_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3646 2461061.8646 13.26 06:39:10.51 +13:11:57.6
199.79132 3.31235 galactic Gem Second-epoch detections are separated by 6.9" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J099.7922+13.1918 | 06:39:10.11 +13:12:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.698+/-0.101 (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 J099.7922+13.1918,2461061.8646,13.26,0.05,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
ATO J099.7922+13.1918 20260121.3646 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/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-05-Q1b1x1_030518_TTUQ1b1x1_14931_hqH9ahqi/fd_Gem-05-Q1b1x1_2026-01-21_02-44-06_20.00sec_-15.00C_LIGHT_0411.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-05-Q1b1x1_030518_TTUQ1b1x1_14931_hqH9ahqi/fd_Gem-05-Q1b1x1_2026-01-21_02-45-27_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:39:10.51 +13:11:57.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-21_02-45-27_20_00sec_-15_00C_LIGHT_0412_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_2026-01-21_02-44-06_20_00sec_-15_00C_LIGHT_0411_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_2026-01-21_02-45-27_20_00sec_-15_00C_LIGHT_0412_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_2026-01-21_02-44-06_20_00sec_-15_00C_LIGHT_0411_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8646,14.46,0.05,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
target 20260121.3646 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/Gem-05-Q1b1x1_2025-12-23_02-33-07_20.00sec_-15.00C_LIGHT_0437.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-05-Q1b1x1_030518_TTUQ1b1x1_14931_hqH9ahqi/fd_Gem-05-Q1b1x1_2026-01-21_02-44-06_20.00sec_-15.00C_LIGHT_0411.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-05-Q1b1x1_030518_TTUQ1b1x1_14931_hqH9ahqi/fd_Gem-05-Q1b1x1_2026-01-21_02-45-27_20.00sec_-15.00C_LIGHT_0412.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:35.72 +11:13:45.5 ;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_Gem-05-Q1b1x1_2025-12-23_02-33-07_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Gem-05-Q1b1x1_2026-01-21_02-45-27_20_00sec_-15_00C_LIGHT_0412_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_2026-01-21_02-44-06_20_00sec_-15_00C_LIGHT_0411_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_2026-01-21_02-45-27_20_00sec_-15_00C_LIGHT_0412_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_2026-01-21_02-44-06_20_00sec_-15_00C_LIGHT_0411_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2073 2461061.7073 14.01 05:41:43.89 -01:45:30.0
206.40035 -16.28425 galactic Ori Second-epoch detections are separated by 8.7" 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 | ATO J085.4369-01.7579 | 05:41:43.89 -01:45:30.0 (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 21.2073* 05 41 43.89 -01 45 30.0 14.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.4369-01.7579,2461061.7073,14.01,0.05,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
ATO J085.4369-01.7579 20260121.2073 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Ori-06-Q1b1x1_000721_TTUQ1b1x1_4829_z1qW3ZrW/fd_Ori-06-Q1b1x1_2026-01-20_22-57-52_20.00sec_-14.90C_LIGHT_0215.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-06-Q1b1x1_000721_TTUQ1b1x1_4829_z1qW3ZrW/fd_Ori-06-Q1b1x1_2026-01-20_22-58-46_20.00sec_-14.90C_LIGHT_0216.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:43.89 -01:45:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-06-Q1b1x1_2025-12-23_00-51-32_20_00sec_-15_00C_LIGHT_0338_fits__*pix.png resample_wcs_fd_Ori-06-Q1b1x1_2026-01-20_22-58-46_20_00sec_-14_90C_LIGHT_0216_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_2026-01-20_22-57-52_20_00sec_-14_90C_LIGHT_0215_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_2026-01-20_22-58-46_20_00sec_-14_90C_LIGHT_0216_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_2026-01-20_22-57-52_20_00sec_-14_90C_LIGHT_0215_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3012 2461061.8012 13.71 05:16:01.72 +46:02:48.9
162.48204 4.50093 galactic Aur Second-epoch detections are separated by 7.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:16:01.72 +46:02:48.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8012,13.71,0.05,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 20260121.3012 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/Aur-02-Q1b1x1_2025-12-23_02-30-08_20.00sec_-15.00C_LIGHT_0433.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-02-Q1b1x1_032445_TTUQ1b1x1_12824_ctmmqbOv/fd_Aur-02-Q1b1x1_2026-01-20_23-11-45_20.00sec_-15.00C_LIGHT_0229.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-02-Q1b1x1_032445_TTUQ1b1x1_12824_ctmmqbOv/fd_Aur-02-Q1b1x1_2026-01-21_03-15-26_20.00sec_-15.00C_LIGHT_0442.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:01.72 +46:02:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-21_03-15-26_20_00sec_-15_00C_LIGHT_0442_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_2026-01-20_23-11-45_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-21_03-15-26_20_00sec_-15_00C_LIGHT_0442_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_2026-01-20_23-11-45_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3298 2461061.8298 13.25 02:32:21.63 +55:42:40.1
136.86885 -4.40570 galactic Per Second-epoch detections are separated by 5.3" 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 | Gaia DR3 457288677002102400 | 02:32:23.21 +55:42:44.6 (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!
TCP 2026 01 21.3298* 02 32 21.63 +55 42 40.1 13.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457288677002102400,2461061.8298,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457288677002102400 20260121.3298 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Per-01-Q1b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20.00sec_-15.00C_LIGHT_0361.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20.00sec_-15.00C_LIGHT_0362.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:21.63 +55:42:40.1 ;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_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3298 2461061.8298 11.94 02:00:01.25 +48:52:49.3
134.38405 -12.46040 galactic Per Second-epoch detections are separated by 1.0" 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 J030.0051+48.8801 | 02:00:01.23 +48:52:48.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.148+/-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!
TCP 2026 01 21.3298* 02 00 01.25 +48 52 49.3 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J030.0051+48.8801,2461061.8298,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J030.0051+48.8801 20260121.3298 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Per-01-Q1b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Per-01-Q1b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20.00sec_-15.00C_LIGHT_0361.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20.00sec_-15.00C_LIGHT_0362.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:00:01.25 +48:52:49.3 ;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_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3298 2461061.8298 12.80 02:04:20.72 +49:26:02.4
134.92238 -11.73286 galactic Per Second-epoch detections are separated by 1.2" 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 | 02:04:20.72 +49:26:02.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.837+/-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!
TCP 2026 01 21.3298* 02 04 20.72 +49 26 02.4 12.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8298,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3298 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/Per-01-Q1b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Per-01-Q1b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20.00sec_-15.00C_LIGHT_0361.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20.00sec_-15.00C_LIGHT_0362.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:20.72 +49:26:02.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3298 2461061.8298 13.15 01:59:31.41 +49:31:01.9
134.12973 -11.86850 galactic Per Second-epoch detections are separated by 1.5" 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 | 01:59:31.41 +49:31:01.9 (user input) | T | P | (position from user input) J-Ks=0.289+/-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 21.3298* 01 59 31.41 +49 31 01.9 13.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8298,13.15,0.05,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 20260121.3298 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/Per-01-Q1b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Per-01-Q1b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20.00sec_-15.00C_LIGHT_0361.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20.00sec_-15.00C_LIGHT_0362.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:31.41 +49:31:01.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3298* 02 00 17.36 +51 48 59.7 13.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8298,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3298 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Per-01-Q1b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Per-01-Q1b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20.00sec_-15.00C_LIGHT_0361.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20.00sec_-15.00C_LIGHT_0362.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:00:17.36 +51:48:59.7 ;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_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3298 2461061.8298 13.02 02:00:50.52 +50:01:17.0
134.20091 -11.32566 galactic Per Second-epoch detections are separated by 1.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:00:50.52 +50:01:17.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.722+/-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 21.3298* 02 00 50.52 +50 01 17.0 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,2461061.8298,13.02,0.05,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
target 20260121.3298 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/Per-01-Q1b1x1_2025-12-23_00-11-37_20.00sec_-14.90C_LIGHT_0292.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Per-01-Q1b1x1_2025-12-23_00-13-11_20.00sec_-15.00C_LIGHT_0294.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20.00sec_-15.00C_LIGHT_0361.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Per-01-Q1b1x1_022139_TTUQ1b1x1_10664_Gtm9UUwp/fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20.00sec_-15.00C_LIGHT_0362.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:00:50.52 +50:01:17.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-55-19_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-01-Q1b1x1_2025-12-23_00-11-37_20_00sec_-14_90C_LIGHT_0292_fits__*pix.png resample_wcs_fd_Per-01-Q1b1x1_2026-01-21_01-54-17_20_00sec_-15_00C_LIGHT_0361_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2190 2461061.7190 14.38 06:59:58.60 +34:05:08.7
182.57586 16.43957 galactic Gem Second-epoch detections are separated by 1.4" 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 J104.9953+34.0835 | 06:59:58.60 +34:05:08.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.9953+34.0835,2461061.7190,14.38,0.05,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 J104.9953+34.0835 20260121.2190 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-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:58.60 +34:05:08.7 ;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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2190 2461061.7190 11.40 06:59:26.40 +37:06:20.6
179.59838 17.44962 galactic Aur Second-epoch detections are separated by 8.6" 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 940887322916961536 | 06:59:27.18 +37:05:53.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5? 1918AnHar..92.....C HD 51560
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 940887322916961536,2461061.7190,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 940887322916961536 20260121.2190 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:26.40 +37:06:20.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2190 2461061.7190 12.02 07:10:53.70 +41:08:22.4
176.37595 20.90531 galactic Aur Second-epoch detections are separated by 0.6" and 4.2 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 949229725656868224 | 07:10:53.68 +41:08:22.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.327+/-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 949229725656868224,2461061.7190,12.02,0.05,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 949229725656868224 20260121.2190 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/Aur-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2025-12-23_02-51-25_20.00sec_-14.90C_LIGHT_0454.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:10:53.70 +41:08:22.4 ;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_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2190 2461061.7190 12.03 05:57:41.68 +32:58:10.8
177.84495 4.28125 galactic Aur Second-epoch detections are separated by 0.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.4225+32.9750 | 05:57:41.79 +32:58:13.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J089.4225+32.9750,2461061.7190,12.03,0.05,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 J089.4225+32.9750 20260121.2190 12.03CV 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/Aur-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2025-12-23_02-51-25_20.00sec_-14.90C_LIGHT_0454.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:41.68 +32:58:10.8 ;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_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2190 2461061.7190 12.15 07:10:57.23 +41:53:11.4
175.61938 21.14892 galactic Aur Second-epoch detections are separated by 0.5" and 4.2 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 949475088549017600 | 07:10:57.15 +41:53:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.732+/-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 949475088549017600,2461061.7190,12.15,0.05,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 949475088549017600 20260121.2190 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/Aur-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2025-12-23_02-51-25_20.00sec_-14.90C_LIGHT_0454.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:10:57.23 +41:53:11.4 ;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_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2190 2461061.7190 12.43 07:12:00.39 +42:09:30.1
175.40633 21.41858 galactic Aur Second-epoch detections are separated by 0.6" and 4.2 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 949575934380366592 | 07:12:00.38 +42:09:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.295+/-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 949575934380366592,2461061.7190,12.43,0.05,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
Gaia DR3 949575934380366592 20260121.2190 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/Aur-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2025-12-23_02-51-25_20.00sec_-14.90C_LIGHT_0454.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:00.39 +42:09:30.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2190 2461061.7190 13.19 06:56:29.69 +42:40:47.5
173.89625 18.87759 galactic Aur Second-epoch detections are separated by 0.6" 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 | ATO J104.1229+42.6796 | 06:56:29.69 +42:40:47.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.409+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.1229+42.6796,2461061.7190,13.19,0.05,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
ATO J104.1229+42.6796 20260121.2190 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/Aur-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2025-12-23_02-51-25_20.00sec_-14.90C_LIGHT_0454.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_014324_TTUQ1b1x1_8387_Iy2lEX3S/fd_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:56:29.69 +42:40:47.5 ;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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_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_2026-01-20_23-15-34_20_00sec_-14_90C_LIGHT_0233_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_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.6974,14.43,0.05,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 20260121.1974 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/Mon-04-Q1b1x1_2025-12-23_00-26-26_20.00sec_-14.90C_LIGHT_0310.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-04-Q1b1x1_001717_TTUQ1b1x1_11256_K773lgfC/fd_Mon-04-Q1b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-04-Q1b1x1_001717_TTUQ1b1x1_11256_K773lgfC/fd_Mon-04-Q1b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:39.53 -07:05:27.4 ;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_Mon-04-Q1b1x1_2025-12-23_00-26-26_20_00sec_-14_90C_LIGHT_0310_fits__*pix.png resample_wcs_fd_Mon-04-Q1b1x1_2026-01-20_22-44-28_20_00sec_-15_00C_LIGHT_0202_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_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_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_2026-01-20_22-44-28_20_00sec_-15_00C_LIGHT_0202_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_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2870 2461061.7870 14.23 08:28:39.39 +73:44:51.7
140.57644 32.70270 galactic Cam Second-epoch detections are separated by 3.6" 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 | Large-amplitude variable Gaia DR2 1123221397734593536 | 08:28:39.39 +73:44:51.7 (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)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1123221397734593536,2461061.7870,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1123221397734593536 20260121.2870 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2025-12-23_04-16-13_20.00sec_-15.00C_LIGHT_0542.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-01-Q1b1x1_010917_TTUQ1b1x1_25033_j7lqJ62a/fd_UMa-01-Q1b1x1_2026-01-21_00-52-44_20.00sec_-15.00C_LIGHT_0315.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-01-Q1b1x1_010917_TTUQ1b1x1_25033_j7lqJ62a/fd_UMa-01-Q1b1x1_2026-01-21_00-53-25_20.00sec_-15.00C_LIGHT_0316.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:28:39.39 +73:44:51.7 ;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_UMa-01-Q1b1x1_2025-12-23_04-16-13_20_00sec_-15_00C_LIGHT_0542_fits__*pix.png resample_wcs_fd_UMa-01-Q1b1x1_2026-01-21_00-53-25_20_00sec_-15_00C_LIGHT_0316_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-01-Q1b1x1_2025-12-23_04-16-13_20_00sec_-15_00C_LIGHT_0542_fits__*pix.png resample_wcs_fd_UMa-01-Q1b1x1_2026-01-21_00-52-44_20_00sec_-15_00C_LIGHT_0315_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-01-Q1b1x1_2025-12-23_04-16-13_20_00sec_-15_00C_LIGHT_0542_fits__*pix.png resample_wcs_fd_UMa-01-Q1b1x1_2026-01-21_00-53-25_20_00sec_-15_00C_LIGHT_0316_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-01-Q1b1x1_2025-12-23_04-16-13_20_00sec_-15_00C_LIGHT_0542_fits__*pix.png resample_wcs_fd_UMa-01-Q1b1x1_2026-01-21_00-52-44_20_00sec_-15_00C_LIGHT_0315_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3494 2461061.8494 13.26 06:05:39.15 +08:45:22.1
199.86014 -6.03557 galactic Ori Second-epoch detections are separated by 1.0" and 0.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.4015+08.7517 | 06:05:39.15 +08:45:22.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3494* 06 05 39.15 +08 45 22.1 13.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.4015+08.7517,2461061.8494,13.26,0.05,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
ATO J091.4015+08.7517 20260121.3494 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/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-02-Q1b1x1_023450_TTUQ1b1x1_29127_Rawk8tcb/fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20.00sec_-15.00C_LIGHT_0391.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-02-Q1b1x1_023450_TTUQ1b1x1_29127_Rawk8tcb/fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20.00sec_-14.90C_LIGHT_0392.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:39.15 +08:45:22.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20_00sec_-14_90C_LIGHT_0392_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20_00sec_-14_90C_LIGHT_0392_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3494 2461061.8494 13.95 06:14:48.09 +16:11:55.6
194.39030 -0.50622 galactic Ori Second-epoch detections are separated by 1.1" and 0.8 pix This object is listed in spacecraft.txt 600.4" JWST
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3369906519551387392 | 06:14:50.09 +16:12:29.8 (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 21.3494* 06 14 48.09 +16 11 55.6 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3369906519551387392,2461061.8494,13.95,0.05,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
Gaia DR3 3369906519551387392 20260121.3494 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/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-02-Q1b1x1_023450_TTUQ1b1x1_29127_Rawk8tcb/fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20.00sec_-15.00C_LIGHT_0391.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-02-Q1b1x1_023450_TTUQ1b1x1_29127_Rawk8tcb/fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20.00sec_-14.90C_LIGHT_0392.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:48.09 +16:11:55.6 ;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_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20_00sec_-14_90C_LIGHT_0392_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20_00sec_-14_90C_LIGHT_0392_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8494,14.39,0.05,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 20260121.3494 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/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-02-Q1b1x1_023450_TTUQ1b1x1_29127_Rawk8tcb/fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20.00sec_-15.00C_LIGHT_0391.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-02-Q1b1x1_023450_TTUQ1b1x1_29127_Rawk8tcb/fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20.00sec_-14.90C_LIGHT_0392.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:35.74 +18:27:39.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20_00sec_-14_90C_LIGHT_0392_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-23-14_20_00sec_-14_90C_LIGHT_0392_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20_00sec_-15_00C_LIGHT_0386_fits__*pix.png resample_wcs_fd_Ori-02-Q1b1x1_2026-01-21_02-22-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.9006,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.4006 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/Cam-09-Q1b1x1_2025-12-23_02-00-56_20.00sec_-15.00C_LIGHT_0407.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-09-Q1b1x1_034246_TTUQ1b1x1_30687_vHkjvjSg/fd_Cam-09-Q1b1x1_2026-01-21_03-36-22_20.00sec_-14.90C_LIGHT_0464.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-09-Q1b1x1_034246_TTUQ1b1x1_30687_vHkjvjSg/fd_Cam-09-Q1b1x1_2026-01-21_03-37-05_20.00sec_-14.90C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:44.21 +62:14:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-09-Q1b1x1_2025-12-23_02-00-56_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Cam-09-Q1b1x1_2026-01-21_03-37-05_20_00sec_-14_90C_LIGHT_0465_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_2026-01-21_03-36-22_20_00sec_-14_90C_LIGHT_0464_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_2026-01-21_03-37-05_20_00sec_-14_90C_LIGHT_0465_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_2026-01-21_03-36-22_20_00sec_-14_90C_LIGHT_0464_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.9506,12.27,0.05,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
target 20260121.4506 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-06-Q1b1x1_044952_TTUQ1b1x1_18029_QsacuCXn/fd_Cam-06-Q1b1x1_2026-01-21_04-48-14_20.00sec_-14.90C_LIGHT_0517.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-06-Q1b1x1_044952_TTUQ1b1x1_18029_QsacuCXn/fd_Cam-06-Q1b1x1_2026-01-21_04-49-14_20.00sec_-14.90C_LIGHT_0518.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:08.81 +68:21:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-01-21_04-49-14_20_00sec_-14_90C_LIGHT_0518_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_2026-01-21_04-48-14_20_00sec_-14_90C_LIGHT_0517_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_2026-01-21_04-49-14_20_00sec_-14_90C_LIGHT_0518_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_2026-01-21_04-48-14_20_00sec_-14_90C_LIGHT_0517_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2259 2461061.7259 14.09 05:55:25.48 +51:54:40.0
160.84410 13.06367 galactic Aur Second-epoch detections are separated by 1.1" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 214939065643449216 | 05:55:25.48 +51:54:40.0 (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=1.107+/-0.105 (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 214939065643449216,2461061.7259,14.09,0.05,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
Large-amplitude variable Gaia DR2 214939065643449216 20260121.2259 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2025-12-23_02-22-04_20.00sec_-15.00C_LIGHT_0425.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-01-Q1b1x1_013316_TTUQ1b1x1_12320_VMDTOGxF/fd_Aur-01-Q1b1x1_2026-01-20_23-24-50_20.00sec_-15.00C_LIGHT_0242.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-01-Q1b1x1_013316_TTUQ1b1x1_12320_VMDTOGxF/fd_Aur-01-Q1b1x1_2026-01-20_23-25-29_20.00sec_-15.00C_LIGHT_0243.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:25.48 +51:54:40.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-01-Q1b1x1_2025-12-23_02-22-04_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Aur-01-Q1b1x1_2026-01-20_23-25-29_20_00sec_-15_00C_LIGHT_0243_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-01-Q1b1x1_2025-12-23_02-22-04_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Aur-01-Q1b1x1_2026-01-20_23-24-50_20_00sec_-15_00C_LIGHT_0242_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q1b1x1_2025-12-23_02-22-04_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Aur-01-Q1b1x1_2026-01-20_23-25-29_20_00sec_-15_00C_LIGHT_0243_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-01-Q1b1x1_2025-12-23_02-22-04_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Aur-01-Q1b1x1_2026-01-20_23-24-50_20_00sec_-15_00C_LIGHT_0242_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3632 2461061.8632 13.89 06:47:29.95 +25:06:01.0
189.91589 10.34528 galactic Gem 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 | Gaia DR3 3381496063598926720 | 06:47:32.03 +25:06:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3381496063598926720,2461061.8632,13.89,0.05,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
Gaia DR3 3381496063598926720 20260121.3632 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-03-Q1b1x1_2025-12-23_02-10-23_20.00sec_-14.90C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-03-Q1b1x1_030135_TTUQ1b1x1_2856_ID0WmKpi/fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20.00sec_-15.00C_LIGHT_0409.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-03-Q1b1x1_030135_TTUQ1b1x1_2856_ID0WmKpi/fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20.00sec_-15.00C_LIGHT_0410.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:47:29.95 +25:06:01.0 ;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_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20_00sec_-15_00C_LIGHT_0410_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20_00sec_-15_00C_LIGHT_0409_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20_00sec_-15_00C_LIGHT_0410_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20_00sec_-15_00C_LIGHT_0409_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3632 2461061.8632 14.38 06:36:11.84 +26:16:37.4
187.72288 8.55975 galactic Gem Second-epoch detections are separated by 7.4" 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 3384159527437756032 | 06:36:09.92 +26:17:02.5 (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 3384159527437756032,2461061.8632,14.38,0.05,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 3384159527437756032 20260121.3632 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-03-Q1b1x1_2025-12-23_02-10-23_20.00sec_-14.90C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-03-Q1b1x1_030135_TTUQ1b1x1_2856_ID0WmKpi/fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20.00sec_-15.00C_LIGHT_0409.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-03-Q1b1x1_030135_TTUQ1b1x1_2856_ID0WmKpi/fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20.00sec_-15.00C_LIGHT_0410.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:11.84 +26:16:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20_00sec_-15_00C_LIGHT_0410_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20_00sec_-15_00C_LIGHT_0409_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20_00sec_-15_00C_LIGHT_0410_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20_00sec_-15_00C_LIGHT_0409_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3632 2461061.8632 13.22 06:32:50.45 +21:12:47.8
191.94193 5.60920 galactic Gem Second-epoch detections are separated by 0.8" 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 J098.2143+21.2124 | 06:32:50.45 +21:12:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.694+/-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
ATO J098.2143+21.2124,2461061.8632,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.2143+21.2124 20260121.3632 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-03-Q1b1x1_2025-12-23_02-10-23_20.00sec_-14.90C_LIGHT_0416.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-03-Q1b1x1_2025-12-23_02-11-12_20.00sec_-14.90C_LIGHT_0417.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-03-Q1b1x1_030135_TTUQ1b1x1_2856_ID0WmKpi/fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20.00sec_-15.00C_LIGHT_0409.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-03-Q1b1x1_030135_TTUQ1b1x1_2856_ID0WmKpi/fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20.00sec_-15.00C_LIGHT_0410.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:50.45 +21:12:47.8 ;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-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20_00sec_-15_00C_LIGHT_0410_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20_00sec_-15_00C_LIGHT_0409_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-43-20_20_00sec_-15_00C_LIGHT_0410_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-03-Q1b1x1_2025-12-23_02-10-23_20_00sec_-14_90C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Gem-03-Q1b1x1_2026-01-21_02-42-26_20_00sec_-15_00C_LIGHT_0409_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3582 2461061.8582 12.16 06:56:30.71 +05:43:22.6
208.40823 3.73108 galactic Mon Second-epoch detections are separated by 2.3" 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 3129559565549824128 | 06:56:30.40 +05:43:26.3 (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 3129559565549824128,2461061.8582,12.16,0.05,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 3129559565549824128 20260121.3582 12.16CV 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_2026-01-21_CI_Mon-01-Q1b1x1_023845_TTUQ1b1x1_4972_sS07qIm7/fd_Mon-01-Q1b1x1_2026-01-21_02-35-09_20.00sec_-15.00C_LIGHT_0402.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-01-Q1b1x1_023845_TTUQ1b1x1_4972_sS07qIm7/fd_Mon-01-Q1b1x1_2026-01-21_02-36-04_20.00sec_-15.00C_LIGHT_0403.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:56:30.71 +05:43:22.6 ;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_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-21_02-36-04_20_00sec_-15_00C_LIGHT_0403_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_2026-01-21_02-35-09_20_00sec_-15_00C_LIGHT_0402_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_2026-01-21_02-36-04_20_00sec_-15_00C_LIGHT_0403_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_2026-01-21_02-35-09_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3582 2461061.8582 14.03 06:55:12.89 +01:46:57.0
211.77554 1.65280 galactic Mon Second-epoch detections are separated by 3.4" 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 3114182796656008704 | 06:55:15.52 +01:47:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1949AnHar.112....1C HD 289360
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114182796656008704,2461061.8582,14.03,0.05,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 3114182796656008704 20260121.3582 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/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-01-Q1b1x1_023845_TTUQ1b1x1_4972_sS07qIm7/fd_Mon-01-Q1b1x1_2026-01-21_02-35-09_20.00sec_-15.00C_LIGHT_0402.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-01-Q1b1x1_023845_TTUQ1b1x1_4972_sS07qIm7/fd_Mon-01-Q1b1x1_2026-01-21_02-36-04_20.00sec_-15.00C_LIGHT_0403.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:55:12.89 +01:46:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-21_02-36-04_20_00sec_-15_00C_LIGHT_0403_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_2026-01-21_02-35-09_20_00sec_-15_00C_LIGHT_0402_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_2026-01-21_02-36-04_20_00sec_-15_00C_LIGHT_0403_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_2026-01-21_02-35-09_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3582 2461061.8582 14.32 07:18:15.65 +08:43:48.1
208.13068 9.89997 galactic CMi 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 3155218112494313728 | 07:18:12.72 +08:43:31.5 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3155218112494313728,2461061.8582,14.32,0.05,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
Gaia DR3 3155218112494313728 20260121.3582 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/Mon-01-Q1b1x1_2025-12-23_01-56-57_20.00sec_-15.00C_LIGHT_0403.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-01-Q1b1x1_023845_TTUQ1b1x1_4972_sS07qIm7/fd_Mon-01-Q1b1x1_2026-01-21_02-35-09_20.00sec_-15.00C_LIGHT_0402.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-01-Q1b1x1_023845_TTUQ1b1x1_4972_sS07qIm7/fd_Mon-01-Q1b1x1_2026-01-21_02-36-04_20.00sec_-15.00C_LIGHT_0403.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:18:15.65 +08:43:48.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-01-Q1b1x1_2025-12-23_01-56-57_20_00sec_-15_00C_LIGHT_0403_fits__*pix.png resample_wcs_fd_Mon-01-Q1b1x1_2026-01-21_02-36-04_20_00sec_-15_00C_LIGHT_0403_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_2026-01-21_02-35-09_20_00sec_-15_00C_LIGHT_0402_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_2026-01-21_02-36-04_20_00sec_-15_00C_LIGHT_0403_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_2026-01-21_02-35-09_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7652,12.59,0.05,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
target 20260121.2652 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/Cam-03-Q1b1x1_2025-12-23_01-09-01_20.00sec_-15.00C_LIGHT_0358.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-03-Q1b1x1_005531_TTUQ1b1x1_5542_aSuXcMrD/fd_Cam-03-Q1b1x1_2026-01-21_00-21-18_20.00sec_-14.90C_LIGHT_0293.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cam-03-Q1b1x1_005531_TTUQ1b1x1_5542_aSuXcMrD/fd_Cam-03-Q1b1x1_2026-01-21_00-22-04_20.00sec_-15.00C_LIGHT_0294.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:30.94 +74:57:47.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-03-Q1b1x1_2025-12-23_01-09-01_20_00sec_-15_00C_LIGHT_0358_fits__*pix.png resample_wcs_fd_Cam-03-Q1b1x1_2026-01-21_00-22-04_20_00sec_-15_00C_LIGHT_0294_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-03-Q1b1x1_2025-12-23_01-09-01_20_00sec_-15_00C_LIGHT_0358_fits__*pix.png resample_wcs_fd_Cam-03-Q1b1x1_2026-01-21_00-21-18_20_00sec_-14_90C_LIGHT_0293_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-03-Q1b1x1_2025-12-23_01-09-01_20_00sec_-15_00C_LIGHT_0358_fits__*pix.png resample_wcs_fd_Cam-03-Q1b1x1_2026-01-21_00-22-04_20_00sec_-15_00C_LIGHT_0294_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-03-Q1b1x1_2025-12-23_01-09-01_20_00sec_-15_00C_LIGHT_0358_fits__*pix.png resample_wcs_fd_Cam-03-Q1b1x1_2026-01-21_00-21-18_20_00sec_-14_90C_LIGHT_0293_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4473 2461061.9473 13.77 18:34:42.36 +80:43:51.7
112.50570 27.41849 galactic Dra Second-epoch detections are separated by 1.9" 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 2295833884284528000 | 18:34:36.13 +80:44:28.4 (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 2295833884284528000,2461061.9473,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2295833884284528000 20260121.4473 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/UMi-01-Q1b1x1_2025-12-23_05-21-39_20.00sec_-15.00C_LIGHT_0618.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMi-01-Q1b1x1_044452_TTUQ1b1x1_651_fl4JgB3I/fd_UMi-01-Q1b1x1_2026-01-21_04-43-36_20.00sec_-14.90C_LIGHT_0512.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMi-01-Q1b1x1_044452_TTUQ1b1x1_651_fl4JgB3I/fd_UMi-01-Q1b1x1_2026-01-21_04-44-16_20.00sec_-15.00C_LIGHT_0513.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:34:42.36 +80:43:51.7 ;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_UMi-01-Q1b1x1_2025-12-23_05-21-39_20_00sec_-15_00C_LIGHT_0618_fits__*pix.png resample_wcs_fd_UMi-01-Q1b1x1_2026-01-21_04-44-16_20_00sec_-15_00C_LIGHT_0513_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMi-01-Q1b1x1_2025-12-23_05-21-39_20_00sec_-15_00C_LIGHT_0618_fits__*pix.png resample_wcs_fd_UMi-01-Q1b1x1_2026-01-21_04-43-36_20_00sec_-14_90C_LIGHT_0512_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMi-01-Q1b1x1_2025-12-23_05-21-39_20_00sec_-15_00C_LIGHT_0618_fits__*pix.png resample_wcs_fd_UMi-01-Q1b1x1_2026-01-21_04-44-16_20_00sec_-15_00C_LIGHT_0513_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMi-01-Q1b1x1_2025-12-23_05-21-39_20_00sec_-15_00C_LIGHT_0618_fits__*pix.png resample_wcs_fd_UMi-01-Q1b1x1_2026-01-21_04-43-36_20_00sec_-14_90C_LIGHT_0512_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7815,14.16,0.05,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 20260121.2815 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:51.87 -19:12:33.7 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 13.86 07:23:34.34 -13:45:06.0
228.80353 0.71164 galactic CMa Second-epoch detections are separated by 2.9" 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 3031995466413712128 | 07:23:32.69 -13:44:57.5 (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 3031995466413712128,2461061.7815,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3031995466413712128 20260121.2815 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:23:34.34 -13:45:06.0 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 13.90 07:35:44.30 -16:09:55.3
232.33074 2.13491 galactic Pup Second-epoch detections are separated by 3.2" 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 3027513449006259584 | 07:35:44.79 -16:09:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.387+/- (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3027513449006259584,2461061.7815,13.90,0.05,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 3027513449006259584 20260121.2815 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:35:44.30 -16:09:55.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 13.99 07:26:31.21 -20:59:19.4
235.51059 -2.09900 galactic CMa Second-epoch detections are separated by 1.4" 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 5620235564634114560 | 07:26:28.55 -20:59:42.2 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5620235564634114560,2461061.7815,13.99,0.05,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
Gaia DR3 5620235564634114560 20260121.2815 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:26:31.21 -20:59:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7815,14.04,0.05,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
target 20260121.2815 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:08:45.67 -21:57:53.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7815,13.94,0.05,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 20260121.2815 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:25:39.94 -13:35:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 13.89 07:36:05.78 -13:39:52.9
230.18374 3.42419 galactic Pup Second-epoch detections are separated by 3.1" 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 | GDS_J0736051-133921 | 07:36:05.13 -13:39:21.3 (Gaia DR3) | VAR (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
GDS_J0736051-133921,2461061.7815,13.89,0.05,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
GDS_J0736051-133921 20260121.2815 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:05.78 -13:39:52.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 13.91 07:37:00.36 -13:32:12.6
230.17914 3.67950 galactic Pup Second-epoch detections are separated by 3.8" 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 | ATO J114.2489-13.5392 | 07:37:00.36 -13:32:12.6 (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 J114.2489-13.5392,2461061.7815,13.91,0.05,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 J114.2489-13.5392 20260121.2815 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:00.36 -13:32:12.6 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 14.24 07:34:40.52 -22:12:21.6
237.48898 -1.02010 galactic Pup Second-epoch detections are separated by 1.1" 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 | 07:34:40.52 -22:12:21.6 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7815,14.24,0.05,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
target 20260121.2815 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:34:40.52 -22:12:21.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 14.18 07:14:32.39 -23:08:56.4
236.13060 -5.56120 galactic CMa Second-epoch detections are separated by 3.3" 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 | ATO J108.6444-23.1533 | 07:14:34.67 -23:09:12.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.6444-23.1533,2461061.7815,14.18,0.05,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 J108.6444-23.1533 20260121.2815 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:32.39 -23:08:56.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 14.27 07:22:40.72 -22:49:55.2
236.71762 -3.75383 galactic CMa Second-epoch detections are separated by 4.4" 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 J110.6655-22.8403 | 07:22:40.30 -22:50:40.6 (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 J110.6655-22.8403,2461061.7815,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.6655-22.8403 20260121.2815 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:22:40.72 -22:49:55.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 14.23 07:21:41.72 -23:01:58.3
236.78953 -4.04786 galactic CMa Second-epoch detections are separated by 2.6" 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 J110.4266-23.0453 | 07:21:41.72 -23:01:58.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.4266-23.0453,2461061.7815,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.4266-23.0453 20260121.2815 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:21:41.72 -23:01:58.3 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2815 2461061.7815 14.24 07:25:27.47 -14:29:57.7
229.67861 0.76026 galactic CMa Second-epoch detections are separated by 2.0" 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 | ATO J111.3630-14.4994 | 07:25:27.47 -14:29:57.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J111.3630-14.4994,2461061.7815,14.24,0.05,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 J111.3630-14.4994 20260121.2815 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:25:27.47 -14:29:57.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.7815,14.39,0.05,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 20260121.2815 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20.00sec_-15.00C_LIGHT_0308.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_020136_TTUQ1b1x1_26252_vDZwnDkU/fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:21:29.83 -22:19:37.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-45-45_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_00-44-39_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 10.31 22:40:08.72 +65:26:22.7
109.83916 5.96164 galactic Cep Second-epoch detections are separated by 0.3" 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 2212429536409446528 | 22:40:08.77 +65:26:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.042 (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 2212429536409446528,2461061.8333,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212429536409446528 20260121.3333 10.31CV 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:40:08.72 +65:26:22.7 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 11.61 22:47:59.99 +66:31:44.6
111.06532 6.54431 galactic Cep Second-epoch detections are separated by 0.3" 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 2212593398001737344 | 22:47:59.96 +66:31:44.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-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
Gaia DR3 2212593398001737344,2461061.8333,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212593398001737344 20260121.3333 11.61CV 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:47:59.99 +66:31:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 11.73 22:40:55.71 +64:54:30.8
109.65340 5.45702 galactic Cep 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 2211606448878161024 | 22:40:54.87 +64:54:28.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M:V 1956AJ.....61..201V MCC 846
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2211606448878161024,2461061.8333,11.73,0.05,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 2211606448878161024 20260121.3333 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:40:55.71 +64:54:30.8 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 11.15 22:41:35.81 +64:44:47.6
109.63774 5.28080 galactic Cep Second-epoch detections are separated by 0.3" 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 | Gaia DR3 2211589715687541888 | 22:41:35.60 +64:44:45.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.249+/-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 2211589715687541888,2461061.8333,11.15,0.05,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 2211589715687541888 20260121.3333 11.15CV 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:41:35.81 +64:44:47.6 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 10.82 22:52:55.36 +66:23:24.8
111.44373 6.19870 galactic Cep Second-epoch detections are separated by 0.5" 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 2212204308326033152 | 22:52:55.27 +66:23:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.173+/-0.037 (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 2212204308326033152,2461061.8333,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2212204308326033152 20260121.3333 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-22_22-25-37_20.00sec_-14.90C_LIGHT_0173.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:52:55.36 +66:23:24.8 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8333,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3333 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:35:32.66 +65:19:21.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8333,13.67,0.05,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 20260121.3333 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:40:56.94 +70:23:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 12.67 22:41:10.80 +66:22:11.5
110.38487 6.72472 galactic Cep Second-epoch detections are separated by 1.6" 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 | target | 22:41:10.80 +66:22:11.5 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8333,12.67,0.05,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 20260121.3333 12.67CV 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:41:10.80 +66:22:11.5 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 12.73 22:46:16.54 +66:26:45.3
110.87315 6.55011 galactic Cep Second-epoch detections are separated by 1.2" 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 2212616315948453376 | 22:46:16.55 +66:26:45.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-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
Gaia DR3 2212616315948453376,2461061.8333,12.73,0.05,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 2212616315948453376 20260121.3333 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:46:16.54 +66:26:45.3 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 12.76 22:41:05.45 +65:35:20.0
109.99795 6.04491 galactic Cep Second-epoch detections are separated by 0.4" 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 | target | 22:41:05.45 +65:35:20.0 (user input) | T | P | (position from user input) J-Ks=0.283+/-0.038 (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,2461061.8333,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3333 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:41:05.45 +65:35:20.0 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 12.96 22:50:35.58 +65:49:14.0
110.97579 5.79424 galactic Cep Second-epoch detections are separated by 1.7" 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 | target | 22:50:35.58 +65:49:14.0 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8333,12.96,0.05,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 20260121.3333 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:50:35.58 +65:49:14.0 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3333 2461061.8333 13.43 22:47:48.61 +66:23:47.6
110.98709 6.43535 galactic Cep Second-epoch detections are separated by 3.2" 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 2212588828156589184 | 22:47:47.91 +66:23:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3.5 2015ApJS..220...16T 2MASS J22474714+6623374
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2212588828156589184,2461061.8333,13.43,0.05,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
Gaia DR3 2212588828156589184 20260121.3333 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/Cep-03-Q1b1x1_2025-12-22_22-24-35_20.00sec_-14.90C_LIGHT_0172.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-03-Q1b1x1_021750_TTUQ1b1x1_6664_h5jUV8yH/fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20.00sec_-15.00C_LIGHT_0367.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:47:48.61 +66:23:47.6 ;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_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_02-00-09_20_00sec_-15_00C_LIGHT_0367_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-03-Q1b1x1_2025-12-22_22-24-35_20_00sec_-14_90C_LIGHT_0172_fits__*pix.png resample_wcs_fd_Cep-03-Q1b1x1_2026-01-21_01-59-20_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2395 2461061.7395 13.75 08:09:15.37 +42:44:48.3
177.50589 31.81522 galactic Lyn Second-epoch detections are separated by 0.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:09:15.37 +42:44:48.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.386+/-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
target,2461061.7395,13.75,0.05,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
target 20260121.2395 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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-05-Q1b1x1_014944_TTUQ1b1x1_23913_cXcT8NkB/fd_Lyn-05-Q1b1x1_2026-01-20_23-44-24_20.00sec_-15.00C_LIGHT_0263.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-05-Q1b1x1_014944_TTUQ1b1x1_23913_cXcT8NkB/fd_Lyn-05-Q1b1x1_2026-01-20_23-45-07_20.00sec_-14.90C_LIGHT_0264.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:09:15.37 +42:44:48.3 ;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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-01-20_23-45-07_20_00sec_-14_90C_LIGHT_0264_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-01-20_23-44-24_20_00sec_-15_00C_LIGHT_0263_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-01-20_23-45-07_20_00sec_-14_90C_LIGHT_0264_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-01-20_23-44-24_20_00sec_-15_00C_LIGHT_0263_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3468 2461061.8468 13.29 07:22:49.09 -09:55:12.5
225.33650 2.35596 galactic Mon Second-epoch detections are separated by 2.9" 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 3047541122027092736 | 07:22:46.67 -09:55:27.1 (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 3047541122027092736,2461061.8468,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3047541122027092736 20260121.3468 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-18-42_20.00sec_-14.90C_LIGHT_0386.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:22:49.09 -09:55:12.5 ;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_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_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_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3468 2461061.8468 12.15 07:12:09.99 -14:56:10.5
228.56032 -2.28427 galactic CMa Second-epoch detections are separated by 0.9" 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 | ATO J108.0336-14.9391 | 07:12:08.08 -14:56:21.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.0336-14.9391,2461061.8468,12.15,0.05,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
ATO J108.0336-14.9391 20260121.3468 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/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-18-42_20.00sec_-14.90C_LIGHT_0386.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:09.99 -14:56:10.5 ;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_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_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_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8468,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3468 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/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-18-42_20.00sec_-14.90C_LIGHT_0386.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:13:00.37 -15:06:41.1 ;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_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_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_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3468 2461061.8468 13.32 08:10:00.60 -05:06:28.2
226.81826 14.91542 galactic Mon Second-epoch detections are separated by 2.0" 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 | 08:10:00.60 -05:06:28.2 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.340+/-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
target,2461061.8468,13.32,0.05,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
target 20260121.3468 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/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-40-07_20.00sec_-15.00C_LIGHT_0391.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-18-42_20.00sec_-14.90C_LIGHT_0386.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:00.60 -05:06:28.2 ;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_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_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_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3468 2461061.8468 12.88 07:12:23.26 -14:19:31.4
228.04289 -1.95465 galactic CMa Second-epoch detections are separated by 0.7" 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 | target | 07:12:23.26 -14:19:31.4 (user input) | T | P | (position from user input) J-Ks=0.319+/-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
target,2461061.8468,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3468 12.88CV 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/Mon-06-Q1b1x1_2025-12-23_01-39-17_20.00sec_-15.00C_LIGHT_0390.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Mon-06-Q1b1x1_2025-12-23_01-40-07_20.00sec_-15.00C_LIGHT_0391.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-18-42_20.00sec_-14.90C_LIGHT_0386.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-06-Q1b1x1_024446_TTUQ1b1x1_15849_fYxdhSVC/fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:23.26 -14:19:31.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-06-Q1b1x1_2025-12-23_01-39-17_20_00sec_-15_00C_LIGHT_0390_fits__*pix.png resample_wcs_fd_Mon-06-Q1b1x1_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_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_2026-01-21_02-19-37_20_00sec_-15_00C_LIGHT_0387_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_2026-01-21_02-18-42_20_00sec_-14_90C_LIGHT_0386_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3183 2461061.8183 13.72 08:04:35.80 -29:56:05.9
247.55574 0.83044 galactic Pup Second-epoch detections are separated by 5.5" 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 5596661760458615680 | 08:04:34.86 -29:56:44.9 (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 5596661760458615680,2461061.8183,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5596661760458615680 20260121.3183 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:35.80 -29:56:05.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8183,13.97,0.05,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 20260121.3183 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:54.54 -28:49:11.7 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3183 2461061.8183 13.86 08:11:08.88 -22:46:55.7
242.30742 5.91776 galactic Pup Second-epoch detections are separated by 1.7" 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 | ASAS J081109-2246.2 | 08:11:08.77 -22:46:12.4 (Gaia DR3) | MISC (local) | 2452201.60000 (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J081109-2246.2,2461061.8183,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081109-2246.2 20260121.3183 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:08.88 -22:46:55.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3183 2461061.8183 13.93 08:10:37.57 -26:10:46.9
245.10830 3.97568 galactic Pup Second-epoch detections are separated by 0.8" 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 | ATO J122.6579-26.1916 | 08:10:37.57 -26:10:46.9 (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 J122.6579-26.1916,2461061.8183,13.93,0.05,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 J122.6579-26.1916 20260121.3183 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:37.57 -26:10:46.9 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3183 2461061.8183 14.01 09:01:05.45 -22:06:26.2
248.60117 15.68656 galactic Pyx Second-epoch detections are separated by 6.8" 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 | ATO J135.2686-22.1088 | 09:01:05.45 -22:06:26.2 (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 J135.2686-22.1088,2461061.8183,14.01,0.05,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
ATO J135.2686-22.1088 20260121.3183 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:05.45 -22:06:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3183 2461061.8183 11.55 08:04:08.65 -29:48:15.4
247.39283 0.81732 galactic Pup Second-epoch detections are separated by 1.6" 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 J121.0460-29.7997 | 08:04:08.65 -29:48:16.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-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
ATO J121.0460-29.7997,2461061.8183,11.55,0.05,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
ATO J121.0460-29.7997 20260121.3183 11.55CV 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:08.65 -29:48:15.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3183 2461061.8183 12.37 09:11:52.05 -25:54:42.6
253.26632 15.13687 galactic Pyx Second-epoch detections are separated by 0.4" 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 5650001302904327552 | 09:11:52.08 -25:54:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.246+/-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 5650001302904327552,2461061.8183,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5650001302904327552 20260121.3183 12.37CV 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:52.05 -25:54:42.6 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3183 2461061.8183 11.14 09:10:26.47 -21:33:50.1
249.59635 17.71016 galactic Pyx Second-epoch detections are separated by 0.1" 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 | Gaia DR3 5679112286293786240 | 09:10:26.59 -21:33:50.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.877+/-0.035 (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 5679112286293786240,2461061.8183,11.14,0.05,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 5679112286293786240 20260121.3183 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/Pyx-01-Q1b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Pyx-01-Q1b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pyx-01-Q1b1x1_020349_TTUQ1b1x1_11357_7xKgorca/fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:26.47 -21:33:50.1 ;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_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-38-48_20_00sec_-14_90C_LIGHT_0356_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q1b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_fd_Pyx-01-Q1b1x1_2026-01-21_01-37-35_20_00sec_-15_00C_LIGHT_0355_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3368 2461061.8368 14.13 07:14:46.72 -09:45:35.1
224.26836 0.68046 galactic Mon Second-epoch detections are separated by 1.3" 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 J108.6946-09.7620 | 07:14:46.72 -09:45:35.1 (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 J108.6946-09.7620,2461061.8368,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.6946-09.7620 20260121.3368 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-04-32_20.00sec_-15.00C_LIGHT_0372.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20.00sec_-15.00C_LIGHT_0373.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:46.72 -09:45:35.1 ;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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_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_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_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_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_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_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3368 2461061.8368 14.18 07:07:43.44 -13:55:11.5
227.16174 -2.77183 galactic CMa Second-epoch detections are separated by 0.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.9305-13.9075 | 07:07:42.48 -13:54:32.6 (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 J106.9305-13.9075,2461061.8368,14.18,0.05,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 J106.9305-13.9075 20260121.3368 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/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-04-32_20.00sec_-15.00C_LIGHT_0372.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20.00sec_-15.00C_LIGHT_0373.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:07:43.44 -13:55:11.5 ;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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_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_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_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_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_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_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3368 2461061.8368 13.56 06:48:11.46 -07:19:21.4
219.09133 -4.04980 galactic Mon Second-epoch detections are separated by 5.2" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.0522-07.3167 | 06:48:11.34 -07:19:02.2 (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 J102.0522-07.3167,2461061.8368,13.56,0.05,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
ATO J102.0522-07.3167 20260121.3368 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/Mon-05-Q1b1x1_2025-12-23_01-01-56_20.00sec_-14.90C_LIGHT_0350.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-04-32_20.00sec_-15.00C_LIGHT_0372.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20.00sec_-15.00C_LIGHT_0373.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:48:11.46 -07:19:21.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_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_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_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_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_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_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3368 2461061.8368 12.99 07:14:23.44 -05:42:53.7
220.63924 2.47222 galactic Mon Second-epoch detections are separated by 0.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.5948-05.7218 | 07:14:25.30 -05:43:31.6 (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 J108.5948-05.7218,2461061.8368,12.99,0.05,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
ATO J108.5948-05.7218 20260121.3368 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/Mon-05-Q1b1x1_2025-12-23_01-02-44_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-04-32_20.00sec_-15.00C_LIGHT_0372.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20.00sec_-15.00C_LIGHT_0373.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:23.44 -05:42:53.7 ;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-05-Q1b1x1_2025-12-23_01-02-44_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-02-44_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_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_01-02-44_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-05-Q1b1x1_2025-12-23_01-02-44_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3368 2461061.8368 12.99 06:23:49.23 -13:35:50.6
222.11296 -12.19208 galactic CMa Second-epoch detections are separated by 0.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.9555-13.5973 | 06:23:49.23 -13:35:50.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.454+/-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
ATO J095.9555-13.5973,2461061.8368,12.99,0.05,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
ATO J095.9555-13.5973 20260121.3368 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/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_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-04-32_20.00sec_-15.00C_LIGHT_0372.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Mon-05-Q1b1x1_024243_TTUQ1b1x1_29567_dNUL85xO/fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20.00sec_-15.00C_LIGHT_0373.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:49.23 -13:35:50.6 ;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_Mon-05-Q1b1x1_2025-12-23_01-01-56_20_00sec_-14_90C_LIGHT_0350_fits__*pix.png resample_wcs_fd_Mon-05-Q1b1x1_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_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_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_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_2026-01-21_02-05-13_20_00sec_-15_00C_LIGHT_0373_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_2026-01-21_02-04-32_20_00sec_-15_00C_LIGHT_0372_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4777 2461061.9777 14.36 20:20:32.60 +62:07:29.2
96.42586 14.20180 galactic Dra Second-epoch detections are separated by 3.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2243138655655945600 | 20:20:29.76 +62:08:05.8 (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 2243138655655945600,2461061.9777,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2243138655655945600 20260121.4777 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-05-Q1b1x1_052852_TTUQ1b1x1_7717_riMCv7Eb/fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20.00sec_-15.00C_LIGHT_0557.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-05-Q1b1x1_052852_TTUQ1b1x1_7717_riMCv7Eb/fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20.00sec_-15.00C_LIGHT_0558.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:20:32.60 +62:07:29.2 ;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_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20_00sec_-15_00C_LIGHT_0558_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20_00sec_-15_00C_LIGHT_0557_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20_00sec_-15_00C_LIGHT_0558_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20_00sec_-15_00C_LIGHT_0557_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4777 2461061.9777 12.54 20:31:28.56 +60:38:44.6
95.88768 12.29778 galactic Cep Second-epoch detections are separated by 8.8" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J307.8603+60.6509 | 20:31:27.14 +60:38:50.9 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J307.8603+60.6509,2461061.9777,12.54,0.05,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 J307.8603+60.6509 20260121.4777 12.54CV 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/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-05-Q1b1x1_052852_TTUQ1b1x1_7717_riMCv7Eb/fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20.00sec_-15.00C_LIGHT_0557.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-05-Q1b1x1_052852_TTUQ1b1x1_7717_riMCv7Eb/fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20.00sec_-15.00C_LIGHT_0558.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:31:28.56 +60:38:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20_00sec_-15_00C_LIGHT_0558_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20_00sec_-15_00C_LIGHT_0557_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20_00sec_-15_00C_LIGHT_0558_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20_00sec_-15_00C_LIGHT_0557_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.9777,13.60,0.05,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
target 20260121.4777 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-05-Q1b1x1_052852_TTUQ1b1x1_7717_riMCv7Eb/fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20.00sec_-15.00C_LIGHT_0557.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cep-05-Q1b1x1_052852_TTUQ1b1x1_7717_riMCv7Eb/fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20.00sec_-15.00C_LIGHT_0558.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:45.84 +57:50:34.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20_00sec_-15_00C_LIGHT_0558_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20_00sec_-15_00C_LIGHT_0557_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-28-01_20_00sec_-15_00C_LIGHT_0558_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q1b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q1b1x1_2026-01-21_05-27-24_20_00sec_-15_00C_LIGHT_0557_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8318,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3318 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20.00sec_-14.90C_LIGHT_0364.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20.00sec_-15.00C_LIGHT_0365.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:13:00.66 -20:24:06.2 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3318 2461061.8318 13.93 07:12:31.17 -16:54:11.8
230.34677 -3.11622 galactic CMa Second-epoch detections are separated by 8.2" 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 J108.1259-16.9036 | 07:12:32.35 -16:54:22.9 (Gaia DR3) | MSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.1259-16.9036,2461061.8318,13.93,0.05,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 J108.1259-16.9036 20260121.3318 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20.00sec_-14.90C_LIGHT_0364.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20.00sec_-15.00C_LIGHT_0365.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:31.17 -16:54:11.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3318 2461061.8318 14.04 07:09:23.66 -13:59:21.7
227.40977 -2.44369 galactic CMa Second-epoch detections are separated by 3.6" 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 | ATO J107.3426-13.9864 | 07:09:23.66 -13:59:21.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3426-13.9864,2461061.8318,14.04,0.05,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 J107.3426-13.9864 20260121.3318 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20.00sec_-14.90C_LIGHT_0364.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20.00sec_-15.00C_LIGHT_0365.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:09:23.66 -13:59:21.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3318 2461061.8318 14.35 07:04:29.88 -13:04:27.9
226.04981 -3.08264 galactic CMa Second-epoch detections are separated by 5.9" 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 J106.1259-13.0730 | 07:04:29.88 -13:04:27.9 (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 J106.1259-13.0730,2461061.8318,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1259-13.0730 20260121.3318 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20.00sec_-14.90C_LIGHT_0364.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20.00sec_-15.00C_LIGHT_0365.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:04:29.88 -13:04:27.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3318 2461061.8318 12.04 06:37:42.13 -19:59:29.3
229.47334 -11.88734 galactic CMa Second-epoch detections are separated by 0.6" 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 J099.4185-19.9936 | 06:37:42.26 -19:59:31.4 (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 J099.4185-19.9936,2461061.8318,12.04,0.05,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 J099.4185-19.9936 20260121.3318 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20.00sec_-14.90C_LIGHT_0364.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20.00sec_-15.00C_LIGHT_0365.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:42.13 -19:59:29.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3318 2461061.8318 12.41 07:38:16.10 -13:09:26.0
229.99614 4.13234 galactic Pup Second-epoch detections are separated by 0.9" 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 3030748143493332096 | 07:38:16.15 -13:09:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.139+/-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 3030748143493332096,2461061.8318,12.41,0.05,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 3030748143493332096 20260121.3318 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20.00sec_-14.90C_LIGHT_0364.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20.00sec_-15.00C_LIGHT_0365.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:38:16.10 -13:09:26.0 ;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_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3318 2461061.8318 12.47 06:34:26.22 -20:54:48.8
230.00601 -12.96650 galactic CMa Second-epoch detections are separated by 2.1" 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 2938721872101958400 | 06:34:26.41 -20:54:49.1 (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 2938721872101958400,2461061.8318,12.47,0.05,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 2938721872101958400 20260121.3318 12.47CV 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/CMa-02-Q1b1x1_2025-12-23_00-34-15_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/reference_imgs/CMa-02-Q1b1x1_2025-12-23_00-34-56_20.00sec_-15.00C_LIGHT_0319.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20.00sec_-14.90C_LIGHT_0364.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_CMa-02-Q1b1x1_024644_TTUQ1b1x1_25255_lvPtj2z3/fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20.00sec_-15.00C_LIGHT_0365.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:26.22 -20:54:48.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-58-00_20_00sec_-15_00C_LIGHT_0365_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CMa-02-Q1b1x1_2025-12-23_00-34-15_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png resample_wcs_fd_CMa-02-Q1b1x1_2026-01-21_01-57-16_20_00sec_-14_90C_LIGHT_0364_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3766 2461061.8766 9.60 09:25:06.36 -12:58:15.9
244.86590 25.88462 galactic Hya Second-epoch detections are separated by 0.1" and 10.0 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 5737852561135645952 | 09:25:06.00 -12:58:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3V 1972AJ.....77..486U UGP 205
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5737852561135645952,2461061.8766,9.60,0.05,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 5737852561135645952 20260121.3766 9.60CV 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/Hya-07-Q1b1x1_2025-12-23_02-18-00_20.00sec_-15.10C_LIGHT_0421.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_031241_TTUQ1b1x1_19312_LUyukxsw/fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20.00sec_-15.00C_LIGHT_0428.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_031241_TTUQ1b1x1_19312_LUyukxsw/fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:25:06.36 -12:58:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20_00sec_-15_00C_LIGHT_0428_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8766,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3766 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Hya-07-Q1b1x1_2025-12-23_02-18-00_20.00sec_-15.10C_LIGHT_0421.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_031241_TTUQ1b1x1_19312_LUyukxsw/fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20.00sec_-15.00C_LIGHT_0428.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_031241_TTUQ1b1x1_19312_LUyukxsw/fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:21:15.66 -22:43:56.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20_00sec_-15_00C_LIGHT_0428_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8766,14.32,0.05,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 20260121.3766 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/Hya-07-Q1b1x1_2025-12-23_02-18-00_20.00sec_-15.10C_LIGHT_0421.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_031241_TTUQ1b1x1_19312_LUyukxsw/fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20.00sec_-15.00C_LIGHT_0428.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_031241_TTUQ1b1x1_19312_LUyukxsw/fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:39:42.06 -19:50:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20_00sec_-15_00C_LIGHT_0428_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8766,14.47,0.05,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
target 20260121.3766 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/Hya-07-Q1b1x1_2025-12-23_02-18-00_20.00sec_-15.10C_LIGHT_0421.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_031241_TTUQ1b1x1_19312_LUyukxsw/fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20.00sec_-15.00C_LIGHT_0428.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-07-Q1b1x1_031241_TTUQ1b1x1_19312_LUyukxsw/fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:21:32.30 -22:39:21.2 ;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_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-02-43_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-07-Q1b1x1_2025-12-23_02-18-00_20_00sec_-15_10C_LIGHT_0421_fits__*pix.png resample_wcs_fd_Hya-07-Q1b1x1_2026-01-21_03-01-37_20_00sec_-15_00C_LIGHT_0428_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3967 2461061.8967 13.38 09:07:56.31 +49:35:57.3
169.27463 42.13247 galactic UMa Second-epoch detections are separated by 1.0" and 27.0 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 J136.9847+49.5967 | 09:07:56.31 +49:35:57.3 (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 21.3967* 09 07 56.31 +49 35 57.3 13.4 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
ATO J136.9847+49.5967,2461061.8967,13.38,0.05,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 J136.9847+49.5967 20260121.3967 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_01-32-24_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20.00sec_-14.90C_LIGHT_0560.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:56.31 +49:35:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_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_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3967* 08 58 12.42 +48 35 25.5 12.8 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
target,2461061.8967,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3967 12.79CV 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_01-32-24_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20.00sec_-14.90C_LIGHT_0560.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:58:12.42 +48:35:25.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_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_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3967 2461061.8967 12.13 08:53:04.37 +50:12:10.5
168.77219 39.69341 galactic UMa Second-epoch detections are separated by 3.8" and 29.5 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 1016715314125000448 | 08:53:06.28 +50:11:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3967* 08 53 04.37 +50 12 10.5 12.1 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 1016715314125000448,2461061.8967,12.13,0.05,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 1016715314125000448 20260121.3967 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_01-32-24_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20.00sec_-14.90C_LIGHT_0560.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:53:04.37 +50:12:10.5 ;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_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_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_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8967,12.13,0.05,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
target 20260121.3967 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_01-32-24_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20.00sec_-14.90C_LIGHT_0560.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:35.77 +51:01:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_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_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8967,13.75,0.05,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
target 20260121.3967 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_01-32-24_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20.00sec_-14.90C_LIGHT_0560.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:17:00.57 +49:33:12.7 ;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_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_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_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3967 2461061.8967 13.71 09:04:06.50 +51:46:53.0
166.47536 41.25992 galactic UMa Second-epoch detections are separated by 2.9" and 26.2 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 1016529084342204800 | 09:04:10.93 +51:47:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3967* 09 04 06.50 +51 46 53.0 13.7 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 1016529084342204800,2461061.8967,13.71,0.05,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
Gaia DR3 1016529084342204800 20260121.3967 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/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_01-32-24_20.00sec_-15.00C_LIGHT_0351.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Lyn-02-Q1b1x1_053022_TTUQ1b1x1_30872_D1dBCXI7/fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20.00sec_-14.90C_LIGHT_0560.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:06.50 +51:46:53.0 ;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_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_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_2026-01-21_05-29-40_20_00sec_-14_90C_LIGHT_0560_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_2026-01-21_01-32-24_20_00sec_-15_00C_LIGHT_0351_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3054 2461061.8054 14.48 06:31:50.99 +32:29:42.8
181.63126 10.42153 galactic Aur Second-epoch detections are separated by 6.1" and 7885.9 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 J097.9637+32.4951 | 06:31:50.99 +32:29:42.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.9637+32.4951,2461061.8054,14.48,0.05,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 J097.9637+32.4951 20260121.3054 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-01-Q1b1x1_2025-12-23_02-54-13_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_032846_TTUQ1b1x1_8825_Y1pRnztu/fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20.00sec_-14.90C_LIGHT_0236.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_032846_TTUQ1b1x1_8825_Y1pRnztu/fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20.00sec_-14.90C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:50.99 +32:29:42.8 ;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_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20_00sec_-14_90C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20_00sec_-14_90C_LIGHT_0236_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20_00sec_-14_90C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20_00sec_-14_90C_LIGHT_0236_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3054 2461061.8054 13.71 06:47:00.71 +25:06:02.1
189.86776 10.24563 galactic Gem Second-epoch detections are separated by 3.8" and 6858.7 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 3384493190559039616 | 06:47:00.59 +25:06:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3384493190559039616,2461061.8054,13.71,0.05,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
Gaia DR3 3384493190559039616 20260121.3054 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/Gem-01-Q1b1x1_2025-12-23_02-54-13_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_032846_TTUQ1b1x1_8825_Y1pRnztu/fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20.00sec_-14.90C_LIGHT_0236.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_032846_TTUQ1b1x1_8825_Y1pRnztu/fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20.00sec_-14.90C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:47:00.71 +25:06:02.1 ;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_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20_00sec_-14_90C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20_00sec_-14_90C_LIGHT_0236_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20_00sec_-14_90C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20_00sec_-14_90C_LIGHT_0236_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3054 2461061.8054 14.49 06:47:08.36 +33:28:32.4
182.08695 13.74434 galactic Gem Second-epoch detections are separated by 3.7" and 5340.9 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 938483442605496832 | 06:47:10.42 +33:28:42.3 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 938483442605496832,2461061.8054,14.49,0.05,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
Gaia DR3 938483442605496832 20260121.3054 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/Gem-01-Q1b1x1_2025-12-23_02-54-13_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_032846_TTUQ1b1x1_8825_Y1pRnztu/fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20.00sec_-14.90C_LIGHT_0236.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_032846_TTUQ1b1x1_8825_Y1pRnztu/fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20.00sec_-14.90C_LIGHT_0447.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:47:08.36 +33:28:32.4 ;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_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20_00sec_-14_90C_LIGHT_0447_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20_00sec_-14_90C_LIGHT_0236_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-20-24_20_00sec_-14_90C_LIGHT_0447_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-20_23-18-41_20_00sec_-14_90C_LIGHT_0236_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3779 2461061.8779 14.14 08:50:32.90 -12:39:33.3
239.09315 19.34918 galactic Hya Second-epoch detections are separated by 4.0" 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 | Gaia DR3 5735242006999523840 | 08:50:35.50 -12:39:20.2 (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 5735242006999523840,2461061.8779,14.14,0.05,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 5735242006999523840 20260121.3779 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/Hya-05-Q1b1x1_2025-12-23_02-37-17_20.00sec_-14.90C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-05-Q1b1x1_031046_TTUQ1b1x1_2782_vYdo94cY/fd_Hya-05-Q1b1x1_2026-01-21_03-03-29_20.00sec_-14.90C_LIGHT_0430.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-05-Q1b1x1_031046_TTUQ1b1x1_2782_vYdo94cY/fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20.00sec_-14.90C_LIGHT_0431.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:50:32.90 -12:39:33.3 ;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_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20_00sec_-14_90C_LIGHT_0431_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_2026-01-21_03-03-29_20_00sec_-14_90C_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_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20_00sec_-14_90C_LIGHT_0431_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_2026-01-21_03-03-29_20_00sec_-14_90C_LIGHT_0430_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8779,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3779 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/Hya-05-Q1b1x1_2025-12-23_02-37-17_20.00sec_-14.90C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-05-Q1b1x1_031046_TTUQ1b1x1_2782_vYdo94cY/fd_Hya-05-Q1b1x1_2026-01-21_03-03-29_20.00sec_-14.90C_LIGHT_0430.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-05-Q1b1x1_031046_TTUQ1b1x1_2782_vYdo94cY/fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20.00sec_-14.90C_LIGHT_0431.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:49.54 -13:07:46.5 ;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_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20_00sec_-14_90C_LIGHT_0431_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_2026-01-21_03-03-29_20_00sec_-14_90C_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_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20_00sec_-14_90C_LIGHT_0431_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_2026-01-21_03-03-29_20_00sec_-14_90C_LIGHT_0430_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8779,14.46,0.05,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
target 20260121.3779 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/Hya-05-Q1b1x1_2025-12-23_02-37-17_20.00sec_-14.90C_LIGHT_0441.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-05-Q1b1x1_031046_TTUQ1b1x1_2782_vYdo94cY/fd_Hya-05-Q1b1x1_2026-01-21_03-03-29_20.00sec_-14.90C_LIGHT_0430.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Hya-05-Q1b1x1_031046_TTUQ1b1x1_2782_vYdo94cY/fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20.00sec_-14.90C_LIGHT_0431.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:08.63 -06:41:30.4 ;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_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20_00sec_-14_90C_LIGHT_0431_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_2026-01-21_03-03-29_20_00sec_-14_90C_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_Hya-05-Q1b1x1_2025-12-23_02-37-17_20_00sec_-14_90C_LIGHT_0441_fits__*pix.png resample_wcs_fd_Hya-05-Q1b1x1_2026-01-21_03-04-36_20_00sec_-14_90C_LIGHT_0431_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_2026-01-21_03-03-29_20_00sec_-14_90C_LIGHT_0430_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4761 2461061.9761 9.80 19:42:19.96 +60:21:52.9
92.56563 17.42214 galactic Dra 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 2239073585069039488 | 19:42:25.90 +60:22:00.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.444+/-0.029 (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 2239073585069039488,2461061.9761,9.80,0.05,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 2239073585069039488 20260121.4761 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/Dra-08-Q1b1x1_2026-01-09_03-33-26_20.00sec_-15.00C_LIGHT_0062.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-08-Q1b1x1_052637_TTUQ1b1x1_32394_gEzkryFb/fd_Dra-08-Q1b1x1_2026-01-21_05-24-50_20.00sec_-15.00C_LIGHT_0554.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-08-Q1b1x1_052637_TTUQ1b1x1_32394_gEzkryFb/fd_Dra-08-Q1b1x1_2026-01-21_05-25-55_20.00sec_-14.90C_LIGHT_0555.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:19.96 +60:21:52.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-08-Q1b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q1b1x1_2026-01-21_05-25-55_20_00sec_-14_90C_LIGHT_0555_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_2026-01-21_05-24-50_20_00sec_-15_00C_LIGHT_0554_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_2026-01-21_05-25-55_20_00sec_-14_90C_LIGHT_0555_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_2026-01-21_05-24-50_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.2158 2461061.7158 11.73 05:14:55.58 +51:01:07.8
158.29036 7.21561 galactic Aur Second-epoch detections are separated by 7.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 262492806108471424 | 05:14:54.41 +51:00:51.7 (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 262492806108471424,2461061.7158,11.73,0.05,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 262492806108471424 20260121.2158 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/Aur-02-Q1b1x1_2025-12-23_02-30-08_20.00sec_-15.00C_LIGHT_0433.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-02-Q1b1x1_013931_TTUQ1b1x1_8292_7wt5Douz/fd_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-02-Q1b1x1_013931_TTUQ1b1x1_8292_7wt5Douz/fd_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:55.58 +51:01:07.8 ;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_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-20_23-10-59_20_00sec_-15_00C_LIGHT_0228_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_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-02-Q1b1x1_2025-12-23_02-30-08_20_00sec_-15_00C_LIGHT_0433_fits__*pix.png resample_wcs_fd_Aur-02-Q1b1x1_2026-01-20_23-10-59_20_00sec_-15_00C_LIGHT_0228_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_2026-01-20_23-10-13_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3903 2461061.8903 14.12 06:46:25.88 +26:22:31.7
188.63811 10.67015 galactic Gem Second-epoch detections are separated by 3.0" 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 | target | 06:46:25.88 +26:22:31.7 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8903,14.12,0.05,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 20260121.3903 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/Gem-01-Q1b1x1_2025-12-23_02-54-13_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_034655_TTUQ1b1x1_6297_HwXVKrjL/fd_Gem-01-Q1b1x1_2026-01-21_03-21-30_20.00sec_-15.00C_LIGHT_0448.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_034655_TTUQ1b1x1_6297_HwXVKrjL/fd_Gem-01-Q1b1x1_2026-01-21_03-22-13_20.00sec_-15.00C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:46:25.88 +26:22:31.7 ;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-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-22-13_20_00sec_-15_00C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-21-30_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-22-13_20_00sec_-15_00C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-21-30_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8903,13.91,0.05,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
target 20260121.3903 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Gem-01-Q1b1x1_2025-12-23_02-54-13_20.00sec_-15.00C_LIGHT_0457.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_034655_TTUQ1b1x1_6297_HwXVKrjL/fd_Gem-01-Q1b1x1_2026-01-21_03-21-30_20.00sec_-15.00C_LIGHT_0448.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-01-Q1b1x1_034655_TTUQ1b1x1_6297_HwXVKrjL/fd_Gem-01-Q1b1x1_2026-01-21_03-22-13_20.00sec_-15.00C_LIGHT_0449.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:08.80 +31:44:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-22-13_20_00sec_-15_00C_LIGHT_0449_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-21-30_20_00sec_-15_00C_LIGHT_0448_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-22-13_20_00sec_-15_00C_LIGHT_0449_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-01-Q1b1x1_2025-12-23_02-54-13_20_00sec_-15_00C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Gem-01-Q1b1x1_2026-01-21_03-21-30_20_00sec_-15_00C_LIGHT_0448_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3698* 05 29 12.45 +17 42 50.5 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8699,14.26,0.05,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 20260121.3699 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/Ori-01-Q1b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-01-Q1b1x1_030249_TTUQ1b1x1_11806_n4xoDwv2/fd_Ori-01-Q1b1x1_2026-01-21_02-51-56_20.00sec_-14.90C_LIGHT_0419.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-01-Q1b1x1_030249_TTUQ1b1x1_11806_n4xoDwv2/fd_Ori-01-Q1b1x1_2026-01-21_02-52-53_20.00sec_-15.00C_LIGHT_0420.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:12.45 +17:42:50.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-01-Q1b1x1_2025-12-23_00-58-27_20_00sec_-14_90C_LIGHT_0346_fits__*pix.png resample_wcs_fd_Ori-01-Q1b1x1_2026-01-21_02-52-53_20_00sec_-15_00C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-01-Q1b1x1_2025-12-23_00-58-27_20_00sec_-14_90C_LIGHT_0346_fits__*pix.png resample_wcs_fd_Ori-01-Q1b1x1_2026-01-21_02-51-56_20_00sec_-14_90C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-01-Q1b1x1_2025-12-23_00-58-27_20_00sec_-14_90C_LIGHT_0346_fits__*pix.png resample_wcs_fd_Ori-01-Q1b1x1_2026-01-21_02-52-53_20_00sec_-15_00C_LIGHT_0420_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-01-Q1b1x1_2025-12-23_00-58-27_20_00sec_-14_90C_LIGHT_0346_fits__*pix.png resample_wcs_fd_Ori-01-Q1b1x1_2026-01-21_02-51-56_20_00sec_-14_90C_LIGHT_0419_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3699 2461061.8699 14.19 05:26:35.98 +13:55:24.2
190.46103 -11.70068 galactic Ori Second-epoch detections are separated by 2.1" 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 3389440172547643520 | 05:26:36.65 +13:54:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G 1931AnHar.100...61C HD 243704
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.3698* 05 26 35.98 +13 55 24.2 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3389440172547643520,2461061.8699,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3389440172547643520 20260121.3699 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ori-01-Q1b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-01-Q1b1x1_030249_TTUQ1b1x1_11806_n4xoDwv2/fd_Ori-01-Q1b1x1_2026-01-21_02-51-56_20.00sec_-14.90C_LIGHT_0419.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-01-Q1b1x1_030249_TTUQ1b1x1_11806_n4xoDwv2/fd_Ori-01-Q1b1x1_2026-01-21_02-52-53_20.00sec_-15.00C_LIGHT_0420.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:35.98 +13:55:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-01-Q1b1x1_2025-12-23_00-58-27_20_00sec_-14_90C_LIGHT_0346_fits__*pix.png resample_wcs_fd_Ori-01-Q1b1x1_2026-01-21_02-52-53_20_00sec_-15_00C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-01-Q1b1x1_2025-12-23_00-58-27_20_00sec_-14_90C_LIGHT_0346_fits__*pix.png resample_wcs_fd_Ori-01-Q1b1x1_2026-01-21_02-51-56_20_00sec_-14_90C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-01-Q1b1x1_2025-12-23_00-58-27_20_00sec_-14_90C_LIGHT_0346_fits__*pix.png resample_wcs_fd_Ori-01-Q1b1x1_2026-01-21_02-52-53_20_00sec_-15_00C_LIGHT_0420_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-01-Q1b1x1_2025-12-23_00-58-27_20_00sec_-14_90C_LIGHT_0346_fits__*pix.png resample_wcs_fd_Ori-01-Q1b1x1_2026-01-21_02-51-56_20_00sec_-14_90C_LIGHT_0419_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 11.87 07:46:22.73 -14:54:03.0
232.48935 4.98839 galactic Pup Second-epoch detections are separated by 0.4" 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 3029345682049832320 | 07:46:25.12 -14:53:38.5 (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 3029345682049832320,2461061.8453,11.87,0.05,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 3029345682049832320 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:22.73 -14:54:03.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 13.97 07:46:45.49 -13:09:41.1
231.01793 5.93106 galactic Pup Second-epoch detections are separated by 6.5" 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 | ATO J116.6868-13.1581 | 07:46:45.49 -13:09:41.1 (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 J116.6868-13.1581,2461061.8453,13.97,0.05,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
ATO J116.6868-13.1581 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:45.49 -13:09:41.1 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 12.91 07:30:23.97 -14:35:17.6
230.32721 1.76894 galactic Pup Second-epoch detections are separated by 5.8" 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 | ATO J112.6091-14.5977 | 07:30:26.06 -14:35:33.9 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J112.6091-14.5977,2461061.8453,12.91,0.05,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 J112.6091-14.5977 20260121.3453 12.91CV 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:30:23.97 -14:35:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 12.84 07:41:55.17 -15:05:09.9
232.11675 3.96077 galactic Pup Second-epoch detections are separated by 2.3" 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 3029150931057187840 | 07:41:52.96 -15:05:06.5 (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 3029150931057187840,2461061.8453,12.84,0.05,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
Gaia DR3 3029150931057187840 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:55.17 -15:05:09.9 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 13.19 07:33:38.38 -22:41:37.8
237.79986 -1.46580 galactic Pup Second-epoch detections are separated by 2.1" 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 | ATO J113.4043-22.6981 | 07:33:38.38 -22:41:37.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J113.4043-22.6981,2461061.8453,13.19,0.05,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
ATO J113.4043-22.6981 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:38.38 -22:41:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 13.47 08:07:20.38 -14:42:13.6
234.91864 9.44932 galactic Pup Second-epoch detections are separated by 7.0" 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 | ASASSN-V J080723.22-144217.2 | 08:07:23.22 -14:42:17.2 (Gaia DR3) | SRS (local) | 2458881.72900 (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 J080723.22-144217.2,2461061.8453,13.47,0.05,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
ASASSN-V J080723.22-144217.2 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:20.38 -14:42:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8453,13.92,0.05,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
target 20260121.3453 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:22:51.97 -21:39:42.1 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8453,14.14,0.05,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
target 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:43.74 -17:57:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 14.13 08:13:45.86 -17:09:50.5
237.86340 9.46057 galactic Pup Second-epoch detections are separated by 1.8" 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 | ATO J123.4401-17.1580 | 08:13:45.86 -17:09:50.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.697+/-0.046 (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 J123.4401-17.1580,2461061.8453,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.4401-17.1580 20260121.3453 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:13:45.86 -17:09:50.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 13.99 08:25:20.66 -20:07:56.9
241.90749 10.13334 galactic Pup Second-epoch detections are separated by 0.9" and 10.1 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 5706566748043776256 | 08:25:17.79 -20:07:48.7 (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 5706566748043776256,2461061.8453,13.99,0.05,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
Gaia DR3 5706566748043776256 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:25:20.66 -20:07:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8453,14.21,0.05,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
target 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:54:07.65 -21:00:36.8 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 14.35 07:56:33.55 -21:51:25.4
239.72936 3.54327 galactic Pup Second-epoch detections are separated by 7.8" 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 | 07:56:33.55 -21:51:25.4 (user input) | 5711475685217747968 (VSX @ VizieR) | DSCT|GDOR|SXPHE (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3,2461061.8453,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 20260121.3453 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:56:33.55 -21:51:25.4 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 12.15 07:27:06.14 -20:37:51.3
235.26025 -1.80929 galactic CMa Second-epoch detections are separated by 0.8" 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 5620318341555095552 | 07:27:06.03 -20:37:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.774+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5620318341555095552,2461061.8453,12.15,0.05,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 5620318341555095552 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Pup-01-Q1b1x1_2025-12-23_01-23-30_20.00sec_-15.00C_LIGHT_0375.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:27:06.14 -20:37:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 12.05 07:27:32.88 -20:21:25.7
235.06905 -1.58721 galactic Pup Second-epoch detections are separated by 1.4" 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 | ATO J111.8870-20.3567 | 07:27:32.89 -20:21:24.1 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.239+/-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
ATO J111.8870-20.3567,2461061.8453,12.05,0.05,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 J111.8870-20.3567 20260121.3453 12.05CV 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Pup-01-Q1b1x1_2025-12-23_01-23-30_20.00sec_-15.00C_LIGHT_0375.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:27:32.88 -20:21:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 11.83 07:28:28.27 -13:42:22.5
229.32860 1.78025 galactic Pup Second-epoch detections are separated by 1.1" 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 3033276260019540864 | 07:28:28.28 -13:42:26.0 (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 3033276260019540864,2461061.8453,11.83,0.05,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
Gaia DR3 3033276260019540864 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Pup-01-Q1b1x1_2025-12-23_01-23-30_20.00sec_-15.00C_LIGHT_0375.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:28:28.27 -13:42:22.5 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3453 2461061.8453 12.71 08:29:27.79 -13:51:23.7
237.11835 14.43097 galactic Hya Second-epoch detections are separated by 0.8" 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 | Gaia DR3 5722901741323928064 | 08:29:27.73 -13:51:24.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-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 5722901741323928064,2461061.8453,12.71,0.05,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 5722901741323928064 20260121.3453 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/Pup-01-Q1b1x1_2025-12-23_01-22-45_20.00sec_-14.90C_LIGHT_0374.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Pup-01-Q1b1x1_2025-12-23_01-23-30_20.00sec_-15.00C_LIGHT_0375.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20.00sec_-15.00C_LIGHT_0384.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Pup-01-Q1b1x1_024847_TTUQ1b1x1_10701_noHJgrJh/fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20.00sec_-14.90C_LIGHT_0385.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:27.79 -13:51:23.7 ;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_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-17-38_20_00sec_-14_90C_LIGHT_0385_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pup-01-Q1b1x1_2025-12-23_01-22-45_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Pup-01-Q1b1x1_2026-01-21_02-16-25_20_00sec_-15_00C_LIGHT_0384_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3876 2461061.8876 13.47 06:35:31.02 +33:00:35.7
181.49408 11.33872 galactic Aur Second-epoch detections are separated by 5.0" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J098.8796+33.0005 | 06:35:28.80 +33:00:24.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.8796+33.0005,2461061.8876,13.47,0.05,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
ATO J098.8796+33.0005 20260121.3876 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/Aur-04-Q1b1x1_2025-12-23_02-50-26_20.00sec_-15.00C_LIGHT_0453.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_032640_TTUQ1b1x1_2621_jC7IUzEb/fd_Aur-04-Q1b1x1_2026-01-21_03-17-24_20.00sec_-14.90C_LIGHT_0444.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-04-Q1b1x1_032640_TTUQ1b1x1_2621_jC7IUzEb/fd_Aur-04-Q1b1x1_2026-01-21_03-18-29_20.00sec_-14.90C_LIGHT_0445.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:31.02 +33:00:35.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-04-Q1b1x1_2025-12-23_02-50-26_20_00sec_-15_00C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Aur-04-Q1b1x1_2026-01-21_03-18-29_20_00sec_-14_90C_LIGHT_0445_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_2026-01-21_03-17-24_20_00sec_-14_90C_LIGHT_0444_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_2026-01-21_03-18-29_20_00sec_-14_90C_LIGHT_0445_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_2026-01-21_03-17-24_20_00sec_-14_90C_LIGHT_0444_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4925 2461061.9925 14.00 16:21:42.37 +55:05:08.9
84.42230 43.12021 galactic Dra Second-epoch detections are separated by 1.1" 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 | ATO J245.4260+55.0861 | 16:21:42.37 +55:05:08.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.750+/-0.136 (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 J245.4260+55.0861,2461061.9925,14.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J245.4260+55.0861 20260121.4925 14.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Dra-10-Q1b1x1_060651_TTUQ1b1x1_17792_FVwbH2pf/fd_Dra-10-Q1b1x1_2026-01-21_05-48-34_20.00sec_-15.00C_LIGHT_0579.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-10-Q1b1x1_060651_TTUQ1b1x1_17792_FVwbH2pf/fd_Dra-10-Q1b1x1_2026-01-21_05-49-25_20.00sec_-15.00C_LIGHT_0580.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:21:42.37 +55:05:08.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-10-Q1b1x1_2026-01-09_03-16-10_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Dra-10-Q1b1x1_2026-01-21_05-49-25_20_00sec_-15_00C_LIGHT_0580_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_2026-01-21_05-48-34_20_00sec_-15_00C_LIGHT_0579_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_2026-01-21_05-49-25_20_00sec_-15_00C_LIGHT_0580_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_2026-01-21_05-48-34_20_00sec_-15_00C_LIGHT_0579_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4925 2461061.9925 13.93 16:19:33.62 +57:36:54.4
87.85549 42.71390 galactic Dra Second-epoch detections are separated by 6.2" 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 J244.8894+57.6151 | 16:19:33.62 +57:36:54.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.950+/-0.156 (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 J244.8894+57.6151,2461061.9925,13.93,0.05,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 J244.8894+57.6151 20260121.4925 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/Dra-10-Q1b1x1_2026-01-09_03-16-10_20.00sec_-15.00C_LIGHT_0044.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-10-Q1b1x1_060651_TTUQ1b1x1_17792_FVwbH2pf/fd_Dra-10-Q1b1x1_2026-01-21_05-48-34_20.00sec_-15.00C_LIGHT_0579.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-10-Q1b1x1_060651_TTUQ1b1x1_17792_FVwbH2pf/fd_Dra-10-Q1b1x1_2026-01-21_05-49-25_20.00sec_-15.00C_LIGHT_0580.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:19:33.62 +57:36:54.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-10-Q1b1x1_2026-01-09_03-16-10_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Dra-10-Q1b1x1_2026-01-21_05-49-25_20_00sec_-15_00C_LIGHT_0580_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_2026-01-21_05-48-34_20_00sec_-15_00C_LIGHT_0579_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_2026-01-21_05-49-25_20_00sec_-15_00C_LIGHT_0580_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_2026-01-21_05-48-34_20_00sec_-15_00C_LIGHT_0579_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3915 2461061.8915 12.13 07:41:42.91 +18:03:31.3
201.86237 18.99525 galactic Gem Second-epoch detections are separated by 1.6" 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 671171348186868352 | 07:41:42.63 +18:03:11.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4IV 1950ApJ...112...48M HD 61787
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 671171348186868352,2461061.8915,12.13,0.05,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 671171348186868352 20260121.3915 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/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-04-Q1b1x1_033041_TTUQ1b1x1_21096_LDhxlJBZ/fd_Gem-04-Q1b1x1_2026-01-21_03-23-14_20.00sec_-15.00C_LIGHT_0450.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-04-Q1b1x1_033041_TTUQ1b1x1_21096_LDhxlJBZ/fd_Gem-04-Q1b1x1_2026-01-21_03-24-02_20.00sec_-14.90C_LIGHT_0451.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:42.91 +18:03:31.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-21_03-24-02_20_00sec_-14_90C_LIGHT_0451_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_2026-01-21_03-23-14_20_00sec_-15_00C_LIGHT_0450_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_2026-01-21_03-24-02_20_00sec_-14_90C_LIGHT_0451_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_2026-01-21_03-23-14_20_00sec_-15_00C_LIGHT_0450_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3915 2461061.8915 13.82 06:55:52.18 +25:21:10.8
190.49308 12.16929 galactic Gem Second-epoch detections are separated by 7.6" 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 3381726857960692224 | 06:55:51.41 +25:21:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3381726857960692224,2461061.8915,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3381726857960692224 20260121.3915 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-01-21_CI_Gem-04-Q1b1x1_033041_TTUQ1b1x1_21096_LDhxlJBZ/fd_Gem-04-Q1b1x1_2026-01-21_03-23-14_20.00sec_-15.00C_LIGHT_0450.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-04-Q1b1x1_033041_TTUQ1b1x1_21096_LDhxlJBZ/fd_Gem-04-Q1b1x1_2026-01-21_03-24-02_20.00sec_-14.90C_LIGHT_0451.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:55:52.18 +25:21:10.8 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-21_03-24-02_20_00sec_-14_90C_LIGHT_0451_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_2026-01-21_03-23-14_20_00sec_-15_00C_LIGHT_0450_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_2026-01-21_03-24-02_20_00sec_-14_90C_LIGHT_0451_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_2026-01-21_03-23-14_20_00sec_-15_00C_LIGHT_0450_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3915 2461061.8915 14.22 07:14:11.86 +24:02:04.8
193.46716 15.44450 galactic Gem Second-epoch detections are separated by 2.4" 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 | 07:14:11.86 +24:02:04.8 (user input) | T | P | (position from user input) SpType: C-H 2016ApJS..226....1J LAMOST J071411.40+240203.1
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8915,14.22,0.05,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 20260121.3915 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/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-04-Q1b1x1_033041_TTUQ1b1x1_21096_LDhxlJBZ/fd_Gem-04-Q1b1x1_2026-01-21_03-23-14_20.00sec_-15.00C_LIGHT_0450.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-04-Q1b1x1_033041_TTUQ1b1x1_21096_LDhxlJBZ/fd_Gem-04-Q1b1x1_2026-01-21_03-24-02_20.00sec_-14.90C_LIGHT_0451.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:11.86 +24:02:04.8 ;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_Gem-04-Q1b1x1_2025-12-23_03-01-54_20_00sec_-15_00C_LIGHT_0462_fits__*pix.png resample_wcs_fd_Gem-04-Q1b1x1_2026-01-21_03-24-02_20_00sec_-14_90C_LIGHT_0451_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_2026-01-21_03-23-14_20_00sec_-15_00C_LIGHT_0450_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_2026-01-21_03-24-02_20_00sec_-14_90C_LIGHT_0451_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_2026-01-21_03-23-14_20_00sec_-15_00C_LIGHT_0450_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3915 2461061.8915 14.45 07:38:12.03 +17:09:08.6
202.38679 17.86597 galactic Gem Second-epoch detections are separated by 4.6" 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 3169097801822398720 | 07:38:14.85 +17:09:11.5 (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 3169097801822398720,2461061.8915,14.45,0.05,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
Gaia DR3 3169097801822398720 20260121.3915 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/Gem-04-Q1b1x1_2025-12-23_03-01-54_20.00sec_-15.00C_LIGHT_0462.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-04-Q1b1x1_033041_TTUQ1b1x1_21096_LDhxlJBZ/fd_Gem-04-Q1b1x1_2026-01-21_03-23-14_20.00sec_-15.00C_LIGHT_0450.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Gem-04-Q1b1x1_033041_TTUQ1b1x1_21096_LDhxlJBZ/fd_Gem-04-Q1b1x1_2026-01-21_03-24-02_20.00sec_-14.90C_LIGHT_0451.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:38:12.03 +17:09:08.6 ;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_2026-01-21_03-24-02_20_00sec_-14_90C_LIGHT_0451_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_2026-01-21_03-23-14_20_00sec_-15_00C_LIGHT_0450_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_2026-01-21_03-24-02_20_00sec_-14_90C_LIGHT_0451_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_2026-01-21_03-23-14_20_00sec_-15_00C_LIGHT_0450_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.5128 2461062.0128 10.77 11:32:06.56 +49:15:33.0
152.24357 63.10996 galactic UMa Second-epoch detections are separated by 0.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 789234158003228160 | 11:32:06.58 +49:15:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.295+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.5128* 11 32 06.56 +49 15 33.0 10.8 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 789234158003228160,2461062.0128,10.77,0.05,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 789234158003228160 20260121.5128 10.77CV 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/UMa-10-Q1b1x1_2025-12-23_05-08-00_20.00sec_-14.90C_LIGHT_0602.fits /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2025-12-23_05-08-55_20.00sec_-14.90C_LIGHT_0603.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-10-Q1b1x1_062626_TTUQ1b1x1_23717_mTHUwGz2/fd_UMa-10-Q1b1x1_2026-01-21_06-17-50_20.00sec_-14.90C_LIGHT_0607.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-10-Q1b1x1_062626_TTUQ1b1x1_23717_mTHUwGz2/fd_UMa-10-Q1b1x1_2026-01-21_06-18-46_20.00sec_-14.90C_LIGHT_0608.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:32:06.56 +49:15:33.0 ;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_UMa-10-Q1b1x1_2025-12-23_05-08-00_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png resample_wcs_fd_UMa-10-Q1b1x1_2026-01-21_06-18-46_20_00sec_-14_90C_LIGHT_0608_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-10-Q1b1x1_2025-12-23_05-08-00_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png resample_wcs_fd_UMa-10-Q1b1x1_2026-01-21_06-17-50_20_00sec_-14_90C_LIGHT_0607_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-10-Q1b1x1_2025-12-23_05-08-00_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png resample_wcs_fd_UMa-10-Q1b1x1_2026-01-21_06-18-46_20_00sec_-14_90C_LIGHT_0608_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-10-Q1b1x1_2025-12-23_05-08-00_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png resample_wcs_fd_UMa-10-Q1b1x1_2026-01-21_06-17-50_20_00sec_-14_90C_LIGHT_0607_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.5128 2461062.0128 11.64 10:06:29.83 +42:41:35.6
176.97424 53.23600 galactic UMa Second-epoch detections are separated by 0.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 808491176446495488 | 10:06:29.82 +42:41:35.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.685+/-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!
TCP 2026 01 21.5128* 10 06 29.83 +42 41 35.6 11.6 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 808491176446495488,2461062.0128,11.64,0.05,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 808491176446495488 20260121.5128 11.64CV 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/UMa-10-Q1b1x1_2025-12-23_05-08-00_20.00sec_-14.90C_LIGHT_0602.fits /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2025-12-23_05-08-55_20.00sec_-14.90C_LIGHT_0603.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-10-Q1b1x1_062626_TTUQ1b1x1_23717_mTHUwGz2/fd_UMa-10-Q1b1x1_2026-01-21_06-17-50_20.00sec_-14.90C_LIGHT_0607.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-10-Q1b1x1_062626_TTUQ1b1x1_23717_mTHUwGz2/fd_UMa-10-Q1b1x1_2026-01-21_06-18-46_20.00sec_-14.90C_LIGHT_0608.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:06:29.83 +42:41:35.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-10-Q1b1x1_2025-12-23_05-08-00_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png resample_wcs_fd_UMa-10-Q1b1x1_2026-01-21_06-18-46_20_00sec_-14_90C_LIGHT_0608_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-10-Q1b1x1_2025-12-23_05-08-00_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png resample_wcs_fd_UMa-10-Q1b1x1_2026-01-21_06-17-50_20_00sec_-14_90C_LIGHT_0607_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-10-Q1b1x1_2025-12-23_05-08-00_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png resample_wcs_fd_UMa-10-Q1b1x1_2026-01-21_06-18-46_20_00sec_-14_90C_LIGHT_0608_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-10-Q1b1x1_2025-12-23_05-08-00_20_00sec_-14_90C_LIGHT_0602_fits__*pix.png resample_wcs_fd_UMa-10-Q1b1x1_2026-01-21_06-17-50_20_00sec_-14_90C_LIGHT_0607_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3404 2461061.8404 13.91 05:53:41.97 +08:45:53.6
198.40804 -8.61406 galactic Ori Second-epoch detections are separated by 3.2" 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 3335504316842142720 | 05:53:41.22 +08:46:08.6 (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 21.3405* 05 53 41.97 +08 45 53.6 13.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3335504316842142720,2461061.8404,13.91,0.05,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 3335504316842142720 20260121.3404 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2025-12-23_01-16-04_20.00sec_-15.00C_LIGHT_0366.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-04-Q1b1x1_023648_TTUQ1b1x1_28909_8GyWg96l/fd_Ori-04-Q1b1x1_2026-01-21_02-09-38_20.00sec_-15.00C_LIGHT_0377.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Ori-04-Q1b1x1_023648_TTUQ1b1x1_28909_8GyWg96l/fd_Ori-04-Q1b1x1_2026-01-21_02-10-30_20.00sec_-14.90C_LIGHT_0378.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:41.97 +08:45:53.6 ;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_Ori-04-Q1b1x1_2025-12-23_01-16-04_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png resample_wcs_fd_Ori-04-Q1b1x1_2026-01-21_02-10-30_20_00sec_-14_90C_LIGHT_0378_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-04-Q1b1x1_2025-12-23_01-16-04_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png resample_wcs_fd_Ori-04-Q1b1x1_2026-01-21_02-09-38_20_00sec_-15_00C_LIGHT_0377_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q1b1x1_2025-12-23_01-16-04_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png resample_wcs_fd_Ori-04-Q1b1x1_2026-01-21_02-10-30_20_00sec_-14_90C_LIGHT_0378_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-04-Q1b1x1_2025-12-23_01-16-04_20_00sec_-15_00C_LIGHT_0366_fits__*pix.png resample_wcs_fd_Ori-04-Q1b1x1_2026-01-21_02-09-38_20_00sec_-15_00C_LIGHT_0377_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4845 2461061.9845 13.81 11:50:45.45 +51:49:28.4
143.64983 62.79378 galactic UMa Second-epoch detections are separated by 3.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:50:45.45 +51:49:28.4 (user input) | T | P | (position from user input) J-Ks=0.821+/-0.226 (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 21.4845* 11 50 45.45 +51 49 28.4 13.8 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
target,2461061.9845,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.4845 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-07-Q1b1x1_2025-12-23_04-47-05_20.00sec_-14.90C_LIGHT_0578.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-07-Q1b1x1_053837_TTUQ1b1x1_14527_no6MN4He/fd_UMa-07-Q1b1x1_2026-01-21_05-36-59_20.00sec_-15.00C_LIGHT_0568.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-07-Q1b1x1_053837_TTUQ1b1x1_14527_no6MN4He/fd_UMa-07-Q1b1x1_2026-01-21_05-37-57_20.00sec_-14.90C_LIGHT_0569.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:50:45.45 +51:49:28.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-07-Q1b1x1_2025-12-23_04-47-05_20_00sec_-14_90C_LIGHT_0578_fits__*pix.png resample_wcs_fd_UMa-07-Q1b1x1_2026-01-21_05-37-57_20_00sec_-14_90C_LIGHT_0569_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-07-Q1b1x1_2025-12-23_04-47-05_20_00sec_-14_90C_LIGHT_0578_fits__*pix.png resample_wcs_fd_UMa-07-Q1b1x1_2026-01-21_05-36-59_20_00sec_-15_00C_LIGHT_0568_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-07-Q1b1x1_2025-12-23_04-47-05_20_00sec_-14_90C_LIGHT_0578_fits__*pix.png resample_wcs_fd_UMa-07-Q1b1x1_2026-01-21_05-37-57_20_00sec_-14_90C_LIGHT_0569_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-07-Q1b1x1_2025-12-23_04-47-05_20_00sec_-14_90C_LIGHT_0578_fits__*pix.png resample_wcs_fd_UMa-07-Q1b1x1_2026-01-21_05-36-59_20_00sec_-15_00C_LIGHT_0568_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4835 2461061.9835 13.69 11:50:45.42 +51:49:28.6
143.64991 62.79369 galactic UMa Second-epoch detections are separated by 2.0" and 1.6 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 | 11:50:45.42 +51:49:28.6 (user input) | T | P | (position from user input) J-Ks=0.821+/-0.226 (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 21.4835* 11 50 45.42 +51 49 28.6 13.7 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
target,2461061.9835,13.69,0.05,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 20260121.4835 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/UMa-07-Q1b1x1_2025-12-23_04-47-05_20.00sec_-14.90C_LIGHT_0578.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-07-Q1b1x1_053707_TTUQ1b1x1_5828_LzhnKwDM/fd_UMa-07-Q1b1x1_2026-01-21_05-35-42_20.00sec_-15.00C_LIGHT_0566.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-07-Q1b1x1_053707_TTUQ1b1x1_5828_LzhnKwDM/fd_UMa-07-Q1b1x1_2026-01-21_05-36-18_20.00sec_-15.00C_LIGHT_0567.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:50:45.42 +51:49:28.6 ;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_UMa-07-Q1b1x1_2025-12-23_04-47-05_20_00sec_-14_90C_LIGHT_0578_fits__*pix.png resample_wcs_fd_UMa-07-Q1b1x1_2026-01-21_05-36-18_20_00sec_-15_00C_LIGHT_0567_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-07-Q1b1x1_2025-12-23_04-47-05_20_00sec_-14_90C_LIGHT_0578_fits__*pix.png resample_wcs_fd_UMa-07-Q1b1x1_2026-01-21_05-35-42_20_00sec_-15_00C_LIGHT_0566_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-07-Q1b1x1_2025-12-23_04-47-05_20_00sec_-14_90C_LIGHT_0578_fits__*pix.png resample_wcs_fd_UMa-07-Q1b1x1_2026-01-21_05-36-18_20_00sec_-15_00C_LIGHT_0567_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-07-Q1b1x1_2025-12-23_04-47-05_20_00sec_-14_90C_LIGHT_0578_fits__*pix.png resample_wcs_fd_UMa-07-Q1b1x1_2026-01-21_05-35-42_20_00sec_-15_00C_LIGHT_0566_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4997 2461061.9997 10.99 20:12:46.76 +51:37:59.1
86.76406 9.52885 galactic Cyg Second-epoch detections are separated by 0.1" 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 2088227637790766976 | 20:12:47.31 +51:37:55.7 (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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2088227637790766976,2461061.9997,10.99,0.05,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 2088227637790766976 20260121.4997 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/Cyg-01-Q1b1x1_2026-01-09_05-29-02_20.00sec_-14.90C_LIGHT_0119.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cyg-01-Q1b1x1_061713_TTUQ1b1x1_5229_rwibZWk6/fd_Cyg-01-Q1b1x1_2026-01-21_05-58-53_20.00sec_-14.90C_LIGHT_0589.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cyg-01-Q1b1x1_061713_TTUQ1b1x1_5229_rwibZWk6/fd_Cyg-01-Q1b1x1_2026-01-21_05-59-49_20.00sec_-14.90C_LIGHT_0590.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:46.76 +51:37:59.1 ;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_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-21_05-59-49_20_00sec_-14_90C_LIGHT_0590_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_2026-01-21_05-58-53_20_00sec_-14_90C_LIGHT_0589_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_2026-01-21_05-59-49_20_00sec_-14_90C_LIGHT_0590_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_2026-01-21_05-58-53_20_00sec_-14_90C_LIGHT_0589_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4997 2461061.9997 9.21 20:26:02.39 +52:42:53.0
88.80987 8.42499 galactic Cyg Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.4936+52.7086 | 20:26:02.33 +52:42:53.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0 1927AnHar.100...33C HD 235233 J-Ks=0.601+/-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 J306.4936+52.7086,2461061.9997,9.21,0.05,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
ATO J306.4936+52.7086 20260121.4997 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/Cyg-01-Q1b1x1_2026-01-09_05-29-02_20.00sec_-14.90C_LIGHT_0119.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Cyg-01-Q1b1x1_2026-01-09_05-29-52_20.00sec_-14.90C_LIGHT_0120.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cyg-01-Q1b1x1_061713_TTUQ1b1x1_5229_rwibZWk6/fd_Cyg-01-Q1b1x1_2026-01-21_05-58-53_20.00sec_-14.90C_LIGHT_0589.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Cyg-01-Q1b1x1_061713_TTUQ1b1x1_5229_rwibZWk6/fd_Cyg-01-Q1b1x1_2026-01-21_05-59-49_20.00sec_-14.90C_LIGHT_0590.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:26:02.39 +52:42:53.0 ;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_Cyg-01-Q1b1x1_2026-01-09_05-29-02_20_00sec_-14_90C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Cyg-01-Q1b1x1_2026-01-21_05-59-49_20_00sec_-14_90C_LIGHT_0590_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_2026-01-21_05-58-53_20_00sec_-14_90C_LIGHT_0589_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_2026-01-21_05-59-49_20_00sec_-14_90C_LIGHT_0590_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_2026-01-21_05-58-53_20_00sec_-14_90C_LIGHT_0589_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4911 2461061.9911 14.47 14:45:48.93 +50:23:40.8
87.60312 58.15479 galactic Boo Second-epoch detections are separated by 5.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J221.4543+50.3940 | 14:45:48.93 +50:23:40.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J221.4543+50.3940,2461061.9911,14.47,0.05,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
ATO J221.4543+50.3940 20260121.4911 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/Dra-09-Q1b1x1_2025-12-23_05-11-49_20.00sec_-15.00C_LIGHT_0606.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-09-Q1b1x1_060142_TTUQ1b1x1_25903_xxf837lF/fd_Dra-09-Q1b1x1_2026-01-21_05-46-32_20.00sec_-15.00C_LIGHT_0577.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Dra-09-Q1b1x1_060142_TTUQ1b1x1_25903_xxf837lF/fd_Dra-09-Q1b1x1_2026-01-21_05-47-27_20.00sec_-15.00C_LIGHT_0578.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:45:48.93 +50:23:40.8 ;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_Dra-09-Q1b1x1_2025-12-23_05-11-49_20_00sec_-15_00C_LIGHT_0606_fits__*pix.png resample_wcs_fd_Dra-09-Q1b1x1_2026-01-21_05-47-27_20_00sec_-15_00C_LIGHT_0578_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_2026-01-21_05-46-32_20_00sec_-15_00C_LIGHT_0577_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_2026-01-21_05-47-27_20_00sec_-15_00C_LIGHT_0578_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_2026-01-21_05-46-32_20_00sec_-15_00C_LIGHT_0577_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3617 2461061.8617 14.49 06:22:19.77 +24:38:54.6
187.76197 5.03169 galactic Gem Second-epoch detections are separated by 1.9" 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 3431743263952363136 | 06:22:20.88 +24:39:36.4 (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 3431743263952363136,2461061.8617,14.49,0.05,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
Gaia DR3 3431743263952363136 20260121.3617 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/Aur-06-Q1b1x1_2025-12-23_02-05-55_20.00sec_-15.00C_LIGHT_0412.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-06-Q1b1x1_025842_TTUQ1b1x1_2883_jzREIUbp/fd_Aur-06-Q1b1x1_2026-01-21_02-40-20_20.00sec_-14.90C_LIGHT_0407.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-06-Q1b1x1_025842_TTUQ1b1x1_2883_jzREIUbp/fd_Aur-06-Q1b1x1_2026-01-21_02-41-08_20.00sec_-15.00C_LIGHT_0408.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:19.77 +24:38:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-06-Q1b1x1_2025-12-23_02-05-55_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png resample_wcs_fd_Aur-06-Q1b1x1_2026-01-21_02-41-08_20_00sec_-15_00C_LIGHT_0408_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-06-Q1b1x1_2025-12-23_02-05-55_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png resample_wcs_fd_Aur-06-Q1b1x1_2026-01-21_02-40-20_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-06-Q1b1x1_2025-12-23_02-05-55_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png resample_wcs_fd_Aur-06-Q1b1x1_2026-01-21_02-41-08_20_00sec_-15_00C_LIGHT_0408_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-06-Q1b1x1_2025-12-23_02-05-55_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png resample_wcs_fd_Aur-06-Q1b1x1_2026-01-21_02-40-20_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3617 2461061.8617 13.30 06:34:27.91 +29:08:17.0
184.94886 9.46870 galactic Aur Second-epoch detections are separated by 4.4" 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 J098.6257+29.1272 | 06:34:27.33 +29:07:35.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.6257+29.1272,2461061.8617,13.30,0.05,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 J098.6257+29.1272 20260121.3617 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/Aur-06-Q1b1x1_2025-12-23_02-05-55_20.00sec_-15.00C_LIGHT_0412.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-06-Q1b1x1_025842_TTUQ1b1x1_2883_jzREIUbp/fd_Aur-06-Q1b1x1_2026-01-21_02-40-20_20.00sec_-14.90C_LIGHT_0407.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-06-Q1b1x1_025842_TTUQ1b1x1_2883_jzREIUbp/fd_Aur-06-Q1b1x1_2026-01-21_02-41-08_20.00sec_-15.00C_LIGHT_0408.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:34:27.91 +29:08:17.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-06-Q1b1x1_2025-12-23_02-05-55_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png resample_wcs_fd_Aur-06-Q1b1x1_2026-01-21_02-41-08_20_00sec_-15_00C_LIGHT_0408_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-06-Q1b1x1_2025-12-23_02-05-55_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png resample_wcs_fd_Aur-06-Q1b1x1_2026-01-21_02-40-20_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-06-Q1b1x1_2025-12-23_02-05-55_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png resample_wcs_fd_Aur-06-Q1b1x1_2026-01-21_02-41-08_20_00sec_-15_00C_LIGHT_0408_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-06-Q1b1x1_2025-12-23_02-05-55_20_00sec_-15_00C_LIGHT_0412_fits__*pix.png resample_wcs_fd_Aur-06-Q1b1x1_2026-01-21_02-40-20_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 21.4878* 12 11 05.10 +50 29 07.3 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.9878,12.93,0.05,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 20260121.4878 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2025-12-23_04-50-23_20.00sec_-14.90C_LIGHT_0582.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-08-Q1b1x1_055119_TTUQ1b1x1_28124_6HnCOy6n/fd_UMa-08-Q1b1x1_2026-01-21_05-41-52_20.00sec_-15.00C_LIGHT_0572.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-08-Q1b1x1_055119_TTUQ1b1x1_28124_6HnCOy6n/fd_UMa-08-Q1b1x1_2026-01-21_05-42-39_20.00sec_-15.00C_LIGHT_0573.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:11:05.10 +50:29:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-08-Q1b1x1_2025-12-23_04-50-23_20_00sec_-14_90C_LIGHT_0582_fits__*pix.png resample_wcs_fd_UMa-08-Q1b1x1_2026-01-21_05-42-39_20_00sec_-15_00C_LIGHT_0573_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-08-Q1b1x1_2025-12-23_04-50-23_20_00sec_-14_90C_LIGHT_0582_fits__*pix.png resample_wcs_fd_UMa-08-Q1b1x1_2026-01-21_05-41-52_20_00sec_-15_00C_LIGHT_0572_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-08-Q1b1x1_2025-12-23_04-50-23_20_00sec_-14_90C_LIGHT_0582_fits__*pix.png resample_wcs_fd_UMa-08-Q1b1x1_2026-01-21_05-42-39_20_00sec_-15_00C_LIGHT_0573_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-08-Q1b1x1_2025-12-23_04-50-23_20_00sec_-14_90C_LIGHT_0582_fits__*pix.png resample_wcs_fd_UMa-08-Q1b1x1_2026-01-21_05-41-52_20_00sec_-15_00C_LIGHT_0572_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.4878 2461061.9878 14.41 11:57:17.28 +49:16:59.2
144.54677 65.51065 galactic UMa Second-epoch detections are separated by 6.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:57:17.28 +49:16:59.2 (user input) | T | P | (position from user input) J-Ks=1.143+/-0.310 (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 21.4878* 11 57 17.28 +49 16 59.2 14.4 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
target,2461061.9878,14.41,0.05,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
target 20260121.4878 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/UMa-08-Q1b1x1_2025-12-23_04-50-23_20.00sec_-14.90C_LIGHT_0582.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-08-Q1b1x1_055119_TTUQ1b1x1_28124_6HnCOy6n/fd_UMa-08-Q1b1x1_2026-01-21_05-41-52_20.00sec_-15.00C_LIGHT_0572.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_UMa-08-Q1b1x1_055119_TTUQ1b1x1_28124_6HnCOy6n/fd_UMa-08-Q1b1x1_2026-01-21_05-42-39_20.00sec_-15.00C_LIGHT_0573.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:57:17.28 +49:16:59.2 ;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_UMa-08-Q1b1x1_2025-12-23_04-50-23_20_00sec_-14_90C_LIGHT_0582_fits__*pix.png resample_wcs_fd_UMa-08-Q1b1x1_2026-01-21_05-42-39_20_00sec_-15_00C_LIGHT_0573_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-08-Q1b1x1_2025-12-23_04-50-23_20_00sec_-14_90C_LIGHT_0582_fits__*pix.png resample_wcs_fd_UMa-08-Q1b1x1_2026-01-21_05-41-52_20_00sec_-15_00C_LIGHT_0572_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-08-Q1b1x1_2025-12-23_04-50-23_20_00sec_-14_90C_LIGHT_0582_fits__*pix.png resample_wcs_fd_UMa-08-Q1b1x1_2026-01-21_05-42-39_20_00sec_-15_00C_LIGHT_0573_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-08-Q1b1x1_2025-12-23_04-50-23_20_00sec_-14_90C_LIGHT_0582_fits__*pix.png resample_wcs_fd_UMa-08-Q1b1x1_2026-01-21_05-41-52_20_00sec_-15_00C_LIGHT_0572_fits__*pix.png animation_v2.gif