Mean magnitude and position on the discovery images:
2026 02 27.4251 2461098.9251 11.12 23:08:50.49 +59:24:27.0
110.20399 -0.90496 galactic Cas Second-epoch detections are separated by 0.3" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J347.1853+59.4070 | 23:08:49.48 +59:24:31.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1955IzKry..14....3B [B55b] 1314
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.4251* 23 08 50.49 +59 24 27.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.1853+59.4070,2461098.9251,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.1853+59.4070 20260227.4251 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:08:50.49 +59:24:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4251 2461098.9251 11.26 23:17:45.11 +59:42:55.1
111.36647 -1.03609 galactic Cas Second-epoch detections are separated by 0.8" and 0.5 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 2010808584535656192 | 23:17:44.20 +59:42:57.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1935BSD...C01....0S BSD 19- 435
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.4251* 23 17 45.11 +59 42 55.1 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2010808584535656192,2461098.9251,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2010808584535656192 20260227.4251 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:17:45.11 +59:42:55.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4251 2461098.9251 11.29 23:14:28.86 +59:54:49.3
111.05415 -0.70312 galactic Cep Second-epoch detections are separated by 0.6" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2013739843882278400 | 23:14:29.80 +59:54:58.6 (Gaia DR3) | (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B7: 1935BSD...C01....0S BSD 19- 317
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2013739843882278400,2461098.9251,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2013739843882278400 20260227.4251 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 /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:14:28.86 +59:54:49.3 ;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_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4251 2461098.9251 10.86 22:39:41.20 +57:04:04.4
105.73385 -1.33808 galactic Cep Second-epoch detections are separated by 1.2" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J339.9300+57.0602 | 22:39:41.27 +57:04:04.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.720+/-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 J339.9300+57.0602,2461098.9251,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J339.9300+57.0602 20260227.4251 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:39:41.20 +57:04:04.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4251 2461098.9251 10.12 22:54:49.99 +56:37:00.0
107.36729 -2.68975 galactic Lac Second-epoch detections are separated by 1.3" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J343.6963+56.6147 | 22:54:50.21 +56:37:00.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K5 1928AnHar.100...49C HD 240111 J-Ks=0.689+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J343.6963+56.6147,2461098.9251,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J343.6963+56.6147 20260227.4251 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:54:49.99 +56:37:00.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4251 2461098.9251 10.60 22:57:37.26 +56:33:34.2
107.68975 -2.90614 galactic Cas Second-epoch detections are separated by 0.6" 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 | Gaia DR3 2009809643868141184 | 22:57:37.15 +56:33:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.4251* 22 57 37.26 +56 33 34.2 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009809643868141184,2461098.9251,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009809643868141184 20260227.4251 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-01-41_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-05_CI_Cep-06-Q2b1x1_124429_TTUQ2b1x1_3555_1vWS6Tdo/fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20.00sec_-15.00C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:57:37.26 +56:33:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-12-17_20_00sec_-15_00C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-02-27_04-11-34_20_00sec_-14_90C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 10.27 22:16:38.75 +41:46:31.9
94.41995 -12.36961 galactic Lac Second-epoch detections are separated by 1.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1958135517929775360 | 22:16:39.18 +41:46:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958135517929775360,2461098.9581,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958135517929775360 20260227.4581 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:38.75 +41:46:31.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 10.68 22:14:37.28 +40:21:14.2
93.26269 -13.31483 galactic Lac Second-epoch detections are separated by 2.6" 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 J333.6465+40.3526 | 22:14:37.83 +40:21:08.4 (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 J333.6465+40.3526,2461098.9581,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J333.6465+40.3526 20260227.4581 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:14:37.28 +40:21:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 10.82 22:11:43.42 +40:39:27.7
92.98431 -12.74730 galactic Lac Second-epoch detections are separated by 1.1" and 2.1 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 1958010414123361408 | 22:11:42.95 +40:39:30.2 (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 1958010414123361408,2461098.9581,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958010414123361408 20260227.4581 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:43.42 +40:39:27.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.16 22:16:19.77 +41:34:57.7
94.25766 -12.49433 galactic Lac Second-epoch detections are separated by 1.0" and 2.1 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 1958109713767686144 | 22:16:20.33 +41:34:53.1 (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 1958109713767686144,2461098.9581,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958109713767686144 20260227.4581 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:19.77 +41:34:57.7 ;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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.21 22:11:59.90 +40:58:02.2
93.21310 -12.52661 galactic Lac Second-epoch detections are separated by 1.3" and 2.1 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 1958023883139218944 | 22:11:59.38 +40:58:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1958023883139218944,2461098.9581,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958023883139218944 20260227.4581 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:59.90 +40:58:02.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.22 22:15:13.03 +41:11:10.8
93.84976 -12.69968 galactic Lac Second-epoch detections are separated by 2.2" 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 1957992650138956928 | 22:15:12.53 +41:11:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.441+/- (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 1957992650138956928,2461098.9581,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1957992650138956928 20260227.4581 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:15:13.03 +41:11:10.8 ;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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.35 22:12:27.21 +40:44:28.8
93.14951 -12.76030 galactic Lac Second-epoch detections are separated by 0.4" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1957965815183008768 | 22:12:26.67 +40:44:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1957965815183008768,2461098.9581,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1957965815183008768 20260227.4581 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:12:27.21 +40:44:28.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.38 22:13:46.73 +40:54:10.0
93.45493 -12.77473 galactic Lac Second-epoch detections are separated by 1.1" 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 1957993955807350144 | 22:13:46.20 +40:54:13.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1957993955807350144,2461098.9581,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1957993955807350144 20260227.4581 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:13:46.73 +40:54:10.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.49 22:16:22.15 +41:36:24.8
94.27804 -12.47870 galactic Lac Second-epoch detections are separated by 1.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1958110091723200896 | 22:16:22.65 +41:36:20.1 (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 1958110091723200896,2461098.9581,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958110091723200896 20260227.4581 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:22.15 +41:36:24.8 ;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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.49 22:16:26.45 +41:39:40.5
94.32107 -12.44170 galactic Lac Second-epoch detections are separated by 3.5" and 1.7 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 1958111088155607552 | 22:16:26.92 +41:39:36.6 (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 1958111088155607552,2461098.9581,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958111088155607552 20260227.4581 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:16:26.45 +41:39:40.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.68 22:02:58.59 +42:34:41.6
92.81298 -10.23097 galactic Lac Second-epoch detections are separated by 0.7" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J330.7401+42.5696 | 22:02:59.13 +42:34:44.5 (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 J330.7401+42.5696,2461098.9581,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J330.7401+42.5696 20260227.4581 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:02:58.59 +42:34:41.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.79 22:11:13.91 +40:50:31.6
93.01775 -12.54328 galactic Lac Second-epoch detections are separated by 0.9" and 2.1 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 1958016255277003776 | 22:11:13.42 +40:50:33.9 (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 1958016255277003776,2461098.9581,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1958016255277003776 20260227.4581 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:13.91 +40:50:31.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 11.23 22:09:35.31 +40:43:36.0
92.69063 -12.45332 galactic Lac Second-epoch detections are separated by 0.8" and 2.1 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 1956523221566857984 | 22:09:34.99 +40:43:37.6 (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 1956523221566857984,2461098.9581,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1956523221566857984 20260227.4581 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:35.31 +40:43:36.0 ;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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 10.54 22:21:09.20 +46:56:01.4
98.03209 -8.54312 galactic Lac Second-epoch detections are separated by 1.2" and 1.5 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 J335.2746+46.9384 | 22:21:09.20 +46:56:03.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.841+/-0.037 (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 J335.2746+46.9384,2461098.9581,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J335.2746+46.9384 20260227.4581 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:09.20 +46:56:01.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4581 2461098.9581 10.31 21:55:46.73 +42:03:04.6
91.41925 -9.82544 galactic Cyg Second-epoch detections are separated by 0.9" and 1.5 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 1960772387332859776 | 21:55:46.67 +42:03:05.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.192+/-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 1960772387332859776,2461098.9581,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1960772387332859776 20260227.4581 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-16-04_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-04-Q2b1x1_2025-12-22_20-17-00_20.00sec_-15.00C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20.00sec_-14.90C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-06_CI_Cyg-04-Q2b1x1_135330_TTUQ2b1x1_17694_tE3IyqPN/fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20.00sec_-15.00C_LIGHT_0255.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:46.73 +42:03:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_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_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-52_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-04-Q2b1x1_2025-12-22_20-16-04_20_00sec_-15_00C_LIGHT_0036_fits__*pix.png resample_wcs_fd_Cyg-04-Q2b1x1_2026-02-27_04-59-09_20_00sec_-14_90C_LIGHT_0254_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.2967 2461118.7967 11.18 01:10:34.43 +66:13:51.8
124.86168 3.43103 galactic Cas 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 525589033648326784 | 01:10:33.59 +66:13:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.2967* 01 10 34.43 +66 13 51.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 525589033648326784,2461118.7967,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 525589033648326784 20260319.2967 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 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2025-12-23_00-01-41_20.00sec_-15.00C_LIGHT_0280.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-01-Q2b1x1_021757_TTUQ2b1x1_30188_fY3FZ06V/fd_Cas-01-Q2b1x1_2026-03-19_02-06-38_20.00sec_-14.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-01-Q2b1x1_021757_TTUQ2b1x1_30188_fY3FZ06V/fd_Cas-01-Q2b1x1_2026-03-19_02-07-31_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:10:34.43 +66:13:51.8 ;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_Cas-01-Q2b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q2b1x1_2026-03-19_02-07-31_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-01-Q2b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q2b1x1_2026-03-19_02-06-38_20_00sec_-14_90C_LIGHT_0000_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-Q2b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q2b1x1_2026-03-19_02-07-31_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-01-Q2b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q2b1x1_2026-03-19_02-06-38_20_00sec_-14_90C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.2967 2461118.7967 11.78 01:18:50.60 +65:16:28.2
125.79485 2.55520 galactic Cas Second-epoch detections are separated by 1.8" 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 524929051797261312 | 01:18:49.55 +65:16:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.2967* 01 18 50.60 +65 16 28.2 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 524929051797261312,2461118.7967,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524929051797261312 20260319.2967 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2025-12-23_00-01-41_20.00sec_-15.00C_LIGHT_0280.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-01-Q2b1x1_021757_TTUQ2b1x1_30188_fY3FZ06V/fd_Cas-01-Q2b1x1_2026-03-19_02-06-38_20.00sec_-14.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cas-01-Q2b1x1_021757_TTUQ2b1x1_30188_fY3FZ06V/fd_Cas-01-Q2b1x1_2026-03-19_02-07-31_20.00sec_-15.00C_LIGHT_0001.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:18:50.60 +65:16:28.2 ;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_Cas-01-Q2b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q2b1x1_2026-03-19_02-07-31_20_00sec_-15_00C_LIGHT_0001_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cas-01-Q2b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q2b1x1_2026-03-19_02-06-38_20_00sec_-14_90C_LIGHT_0000_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-Q2b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q2b1x1_2026-03-19_02-07-31_20_00sec_-15_00C_LIGHT_0001_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cas-01-Q2b1x1_2025-12-23_00-01-41_20_00sec_-15_00C_LIGHT_0280_fits__*pix.png resample_wcs_fd_Cas-01-Q2b1x1_2026-03-19_02-06-38_20_00sec_-14_90C_LIGHT_0000_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 13.54 08:06:07.66 +02:35:56.2
219.29159 17.77738 galactic CMi Second-epoch detections are separated by 1.7" 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 | target | 08:06:07.66 +02:35:56.2 (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,2461118.8100,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3100 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:07.66 +02:35:56.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 13.40 08:04:25.16 -06:44:27.9
227.56436 12.89661 galactic Mon Second-epoch detections are separated by 7.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:04:25.16 -06:44:27.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8100,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3100 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:25.16 -06:44:27.9 ;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_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 12.96 08:05:51.99 +02:33:21.9
219.29960 17.69971 galactic CMi Second-epoch detections are separated by 2.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3090999903220823040 | 08:05:52.54 +02:33:18.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3090999903220823040,2461118.8100,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090999903220823040 20260319.3100 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:51.99 +02:33:21.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 12.93 08:06:50.48 +02:38:29.5
219.33902 17.95498 galactic CMi Second-epoch detections are separated by 3.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3090995745692409216 | 08:06:50.00 +02:38:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3090995745692409216,2461118.8100,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090995745692409216 20260319.3100 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:50.48 +02:38:29.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 12.91 08:07:40.75 +01:59:16.4
220.04917 17.83517 galactic CMi Second-epoch detections are separated by 0.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3090698293436147456 | 08:07:41.22 +01:59:15.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3090698293436147456,2461118.8100,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090698293436147456 20260319.3100 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 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:40.75 +01:59:16.4 ;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-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 13.73 08:33:55.08 -03:45:56.3
228.76689 20.73546 galactic Hya Second-epoch detections are separated by 2.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J128.4761-03.7644 | 08:33:55.08 -03:45:56.3 (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 J128.4761-03.7644,2461118.8100,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J128.4761-03.7644 20260319.3100 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:33:55.08 -03:45:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3100 2461118.8100 11.11 08:11:06.13 -06:53:50.3
228.55900 14.25365 galactic Mon Second-epoch detections are separated by 0.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3063842412688692992 | 08:11:05.98 -06:53:52.1 (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 3063842412688692992,2461118.8100,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3063842412688692992 20260319.3100 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 /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-05-51_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-03-Q2b1x1_2025-12-23_03-06-37_20.00sec_-15.00C_LIGHT_0467.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-03-Q2b1x1_022950_TTUQ2b1x1_18814_Hdet6JTR/fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20.00sec_-15.00C_LIGHT_0022.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:06.13 -06:53:50.3 ;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_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-26-39_20_00sec_-15_00C_LIGHT_0022_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-03-Q2b1x1_2025-12-23_03-05-51_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Hya-03-Q2b1x1_2026-03-19_02-25-52_20_00sec_-15_00C_LIGHT_0021_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8089,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3089 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:32.50 -04:50:29.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8089,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3089 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:23.62 -05:45:26.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8089,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3089 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:12.31 -04:49:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3089 2461118.8089 13.29 08:56:19.66 -05:17:23.8
233.37529 24.66621 galactic Hya Second-epoch detections are separated by 4.1" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5760718997083401088 | 08:56:20.24 -05:17:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5760718997083401088,2461118.8089,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5760718997083401088 20260319.3089 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:56:19.66 -05:17:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3089 2461118.8089 12.87 08:55:32.59 -06:03:13.3
233.95921 24.08439 galactic Hya Second-epoch detections are separated by 1.2" 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 5757649027475822464 | 08:55:33.18 -06:03:15.5 (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 5757649027475822464,2461118.8089,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5757649027475822464 20260319.3089 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:32.59 -06:03:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3089 2461118.8089 14.13 09:52:41.81 -09:39:06.3
247.00075 33.18590 galactic Sex Second-epoch detections are separated by 6.1" 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 | Gaia DR3 3770860412624078080 | 09:52:41.28 -09:38:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3089* 09 52 41.81 -09 39 06.3 14.1 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3770860412624078080,2461118.8089,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3770860412624078080 20260319.3089 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:52:41.81 -09:39:06.3 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 10.66 20:09:13.89 +36:40:15.2
73.75181 1.98528 galactic Cyg Second-epoch detections are separated by 4.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J302.3083+36.6818 | 20:09:14.11 +36:40:20.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8: 1949ApJ...110..478N LF 3b +36 283
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.3083+36.6818,2461098.9862,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J302.3083+36.6818 20260227.4862 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:09:13.89 +36:40:15.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 10.78 20:16:14.20 +36:49:24.2
74.65190 0.89774 galactic Cyg Second-epoch detections are separated by 7.5" 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 | Gaia DR3 2060514447226300928 | 20:16:14.69 +36:49:25.1 (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 2060514447226300928,2461098.9862,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2060514447226300928 20260227.4862 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:14.20 +36:49:24.2 ;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_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.13 20:06:40.69 +36:15:26.9
73.12611 2.19381 galactic Cyg Second-epoch detections are separated by 8.7" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J301.6851+36.2543 | 20:06:41.14 +36:15:30.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1925AnHar.100....1C HD 227709
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.6851+36.2543,2461098.9862,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J301.6851+36.2543 20260227.4862 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:06:40.69 +36:15:26.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.11 19:54:19.28 +33:35:35.0
69.52484 2.94758 galactic Cyg Second-epoch detections are separated by 5.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J298.5851+33.5972 | 19:54:19.59 +33:35:30.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8/9 1958IzKry..19..230N [N58] 77
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.5851+33.5972,2461098.9862,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.5851+33.5972 20260227.4862 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:19.28 +33:35:35.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.36 20:12:30.24 +36:13:51.5
73.74312 1.19376 galactic Cyg Second-epoch detections are separated by 4.1" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2058983377296635776 | 20:12:30.79 +36:13:51.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5 1953ApJ...118...77A LF 3a +36 70
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2058983377296635776,2461098.9862,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2058983377296635776 20260227.4862 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:30.24 +36:13:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.47 20:12:46.20 +35:50:05.8
73.44205 0.93087 galactic Cyg Second-epoch detections are separated by 4.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.1987+35.8405 | 20:12:46.70 +35:50:06.8 (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 J303.1987+35.8405,2461098.9862,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.1987+35.8405 20260227.4862 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:46.20 +35:50:05.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.49 20:15:58.91 +38:21:26.5
75.89758 1.79484 galactic Cyg Second-epoch detections are separated by 5.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.9835+38.3617 | 20:15:59.42 +38:21:26.9 (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 J303.9835+38.3617,2461098.9862,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.9835+38.3617 20260227.4862 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:15:58.91 +38:21:26.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.59 20:15:36.89 +35:43:31.4
73.67037 0.38977 galactic Cyg Second-epoch detections are separated by 7.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2057395441962429440 | 20:15:36.43 +35:43:29.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1926AnHar.100...17C HD 228604
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2057395441962429440,2461098.9862,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2057395441962429440 20260227.4862 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:15:36.89 +35:43:31.4 ;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_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.58 20:16:49.87 +38:03:05.0
75.73670 1.48565 galactic Cyg Second-epoch detections are separated by 5.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.2174+38.0608 | 20:16:50.45 +38:03:08.4 (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 J304.2174+38.0608,2461098.9862,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.2174+38.0608 20260227.4862 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:49.87 +38:03:05.0 ;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_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.61 20:09:45.37 +36:02:48.3
73.28519 1.55728 galactic Cyg Second-epoch detections are separated by 4.4" 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 | Large-amplitude variable Gaia DR2 2059144283945281408 | 20:09:46.00 +36:02:51.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2059144283945281408,2461098.9862,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2059144283945281408 20260227.4862 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 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:09:45.37 +36:02:48.3 ;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_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.4862 2461098.9862 11.46 18:59:36.02 +39:26:53.2
69.76544 15.38188 galactic Lyr Second-epoch detections are separated by 8.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J284.9056+39.4459 | 18:59:35.19 +39:26:48.9 (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 J284.9056+39.4459,2461098.9862,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J284.9056+39.4459 20260227.4862 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q2b1x1_2026-01-18_06-06-30_20.00sec_-14.90C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20.00sec_-14.90C_LIGHT_0281.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-07_CI_Cyg-05-Q2b1x1_055811_TTUQ2b1x1_20093_WPvYxIjf/fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20.00sec_-15.00C_LIGHT_0282.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:59:36.02 +39:26:53.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-40-25_20_00sec_-15_00C_LIGHT_0282_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-05-Q2b1x1_2026-01-18_06-06-30_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Cyg-05-Q2b1x1_2026-02-27_05-39-37_20_00sec_-14_90C_LIGHT_0281_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3137 2461118.8137 12.76 13:09:11.87 -38:44:56.6
306.72107 23.99199 galactic Cen Second-epoch detections are separated by 8.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6141586354611786496 | 13:09:11.39 -38:44:53.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6141586354611786496,2461118.8137,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6141586354611786496 20260319.3137 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-01-Q2b1x1_2026-01-21_03-38-15_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-01-Q2b1x1_023950_TTUQ2b1x1_22348_tCsQO7OF/fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20.00sec_-14.90C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-01-Q2b1x1_023950_TTUQ2b1x1_22348_tCsQO7OF/fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20.00sec_-15.00C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:09:11.87 -38:44:56.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20_00sec_-14_90C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20_00sec_-14_90C_LIGHT_0027_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3137 2461118.8137 12.76 12:23:45.22 -34:37:25.3
296.48951 27.90151 galactic Cen Second-epoch detections are separated by 8.6" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:23:45.22 -34:37:25.3 (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,2461118.8137,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3137 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-01-Q2b1x1_2026-01-21_03-38-15_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-01-Q2b1x1_023950_TTUQ2b1x1_22348_tCsQO7OF/fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20.00sec_-14.90C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-01-Q2b1x1_023950_TTUQ2b1x1_22348_tCsQO7OF/fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20.00sec_-15.00C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:23:45.22 -34:37:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20_00sec_-14_90C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20_00sec_-14_90C_LIGHT_0027_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3137 2461118.8137 13.74 13:04:15.05 -38:17:33.4
305.69461 24.51040 galactic Cen Second-epoch detections are separated by 5.6" and 1.7 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 | 13:04:15.05 -38:17:33.4 (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,2461118.8137,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3137 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-01-Q2b1x1_2026-01-21_03-38-15_20.00sec_-15.00C_LIGHT_0466.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-01-Q2b1x1_023950_TTUQ2b1x1_22348_tCsQO7OF/fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20.00sec_-14.90C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-01-Q2b1x1_023950_TTUQ2b1x1_22348_tCsQO7OF/fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20.00sec_-15.00C_LIGHT_0028.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:04:15.05 -38:17:33.4 ;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_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20_00sec_-14_90C_LIGHT_0027_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-54_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-01-Q2b1x1_2026-01-21_03-38-15_20_00sec_-15_00C_LIGHT_0466_fits__*pix.png resample_wcs_fd_Cen-01-Q2b1x1_2026-03-19_02-31-12_20_00sec_-14_90C_LIGHT_0027_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.7986,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.2986 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-11-Q2b1x1_2026-01-21_03-10-52_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-11-Q2b1x1_023549_TTUQ2b1x1_1816_3G6Hj81C/fd_Hya-11-Q2b1x1_2026-03-19_02-09-21_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-11-Q2b1x1_023549_TTUQ2b1x1_1816_3G6Hj81C/fd_Hya-11-Q2b1x1_2026-03-19_02-10-10_20.00sec_-14.90C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:30.74 -20:40:35.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-11-Q2b1x1_2026-01-21_03-10-52_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Hya-11-Q2b1x1_2026-03-19_02-10-10_20_00sec_-14_90C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-11-Q2b1x1_2026-01-21_03-10-52_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Hya-11-Q2b1x1_2026-03-19_02-09-21_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-11-Q2b1x1_2026-01-21_03-10-52_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Hya-11-Q2b1x1_2026-03-19_02-10-10_20_00sec_-14_90C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-11-Q2b1x1_2026-01-21_03-10-52_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Hya-11-Q2b1x1_2026-03-19_02-09-21_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.2986 2461118.7986 13.23 11:00:11.76 -21:30:09.8
271.18213 34.42059 galactic Crt Second-epoch detections are separated by 1.8" 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 3549865958489537152 | 11:00:12.33 -21:30:12.8 (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 3549865958489537152,2461118.7986,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3549865958489537152 20260319.2986 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-11-Q2b1x1_2026-01-21_03-10-52_20.00sec_-15.00C_LIGHT_0437.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-11-Q2b1x1_023549_TTUQ2b1x1_1816_3G6Hj81C/fd_Hya-11-Q2b1x1_2026-03-19_02-09-21_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-11-Q2b1x1_023549_TTUQ2b1x1_1816_3G6Hj81C/fd_Hya-11-Q2b1x1_2026-03-19_02-10-10_20.00sec_-14.90C_LIGHT_0003.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:00:11.76 -21:30:09.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-11-Q2b1x1_2026-01-21_03-10-52_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Hya-11-Q2b1x1_2026-03-19_02-10-10_20_00sec_-14_90C_LIGHT_0003_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-11-Q2b1x1_2026-01-21_03-10-52_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Hya-11-Q2b1x1_2026-03-19_02-09-21_20_00sec_-15_00C_LIGHT_0002_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-11-Q2b1x1_2026-01-21_03-10-52_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Hya-11-Q2b1x1_2026-03-19_02-10-10_20_00sec_-14_90C_LIGHT_0003_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-11-Q2b1x1_2026-01-21_03-10-52_20_00sec_-15_00C_LIGHT_0437_fits__*pix.png resample_wcs_fd_Hya-11-Q2b1x1_2026-03-19_02-09-21_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3211 2461118.8211 13.96 07:25:55.51 +34:47:43.4
183.84115 21.70141 galactic Gem Second-epoch detections are separated by 5.6" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:25:55.51 +34:47:43.4 (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,2461118.8211,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3211 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:25:55.51 +34:47:43.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3211 2461118.8211 13.78 07:24:49.08 +33:53:49.1
184.67428 21.19338 galactic Gem Second-epoch detections are separated by 1.4" 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 | target | 07:24:49.08 +33:53:49.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8211,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3211 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:24:49.08 +33:53:49.1 ;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-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3211 2461118.8211 13.22 07:24:54.89 +34:46:58.2
183.78208 21.50098 galactic Gem Second-epoch detections are separated by 6.8" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 896808829472041856 | 07:24:54.51 +34:47:03.5 (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 896808829472041856,2461118.8211,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 896808829472041856 20260319.3211 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Gem-02-Q2b1x1_2025-12-23_03-36-27_20.00sec_-15.00C_LIGHT_0502.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20.00sec_-14.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Gem-02-Q2b1x1_024751_TTUQ2b1x1_15820_3wieMlRh/fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20.00sec_-15.00C_LIGHT_0041.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:24:54.89 +34:46:58.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-42-38_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Gem-02-Q2b1x1_2025-12-23_03-36-27_20_00sec_-15_00C_LIGHT_0502_fits__*pix.png resample_wcs_fd_Gem-02-Q2b1x1_2026-03-19_02-41-52_20_00sec_-14_90C_LIGHT_0040_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8060,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3060 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-08-Q2b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:19:19.77 -21:09:53.0 ;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_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8060,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3060 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-08-Q2b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:13:41.16 -22:39:45.5 ;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_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8060,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3060 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-08-Q2b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:18:07.53 -12:57:20.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3060 2461118.8060 13.19 09:17:18.95 -13:48:52.8
244.28041 23.87990 galactic Hya Second-epoch detections are separated by 2.2" 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 | Large-amplitude variable Gaia DR2 5731874756933786240 | 09:17:18.28 -13:48:49.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5731874756933786240,2461118.8060,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 5731874756933786240 20260319.3060 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-08-Q2b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:17:18.95 -13:48:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3060 2461118.8060 12.06 09:15:37.06 -13:29:42.4
243.72673 23.75446 galactic Hya Second-epoch detections are separated by 5.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5732695916026182272 | 09:15:36.65 -13:29:41.3 (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 5732695916026182272,2461118.8060,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5732695916026182272 20260319.3060 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-08-Q2b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:15:37.06 -13:29:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3060 2461118.8060 11.98 09:15:13.77 -15:09:39.2
245.08301 22.64553 galactic Hya Second-epoch detections are separated by 1.6" 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 5731471923361316992 | 09:15:14.50 -15:09:40.9 (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 5731471923361316992,2461118.8060,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5731471923361316992 20260319.3060 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-08-Q2b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:15:13.77 -15:09:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3060 2461118.8060 12.40 09:16:11.77 -13:06:38.3
243.49097 24.10258 galactic Hya Second-epoch detections are separated by 3.5" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5732712786657710976 | 09:16:12.17 -13:06:41.3 (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 5732712786657710976,2461118.8060,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5732712786657710976 20260319.3060 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-08-Q2b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:16:11.77 -13:06:38.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3060 2461118.8060 13.33 09:16:40.45 -13:03:33.0
243.52536 24.22592 galactic Hya Second-epoch detections are separated by 5.5" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5738718048585653120 | 09:16:40.98 -13:03:32.6 (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 5738718048585653120,2461118.8060,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5738718048585653120 20260319.3060 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 /data_ssd/NMW-TexasTech/reference_imgs/Hya-08-Q2b1x1_2025-12-23_03-08-56_20.00sec_-15.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-08-Q2b1x1_023348_TTUQ2b1x1_19629_Xv9uVDXF/fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20.00sec_-15.00C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:16:40.45 -13:03:33.0 ;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_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-20-50_20_00sec_-15_00C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-08-Q2b1x1_2025-12-23_03-08-56_20_00sec_-15_00C_LIGHT_0470_fits__*pix.png resample_wcs_fd_Hya-08-Q2b1x1_2026-03-19_02-19-58_20_00sec_-15_00C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.88 07:01:53.89 +42:50:13.7
174.08936 19.86512 galactic Aur Second-epoch detections are separated by 6.5" 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 | target | 07:01:53.89 +42:50:13.7 (user input) | T | P | (position from user input) J-Ks=2.464+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3222 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:53.89 +42:50:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.82 07:01:14.06 +41:55:54.3
174.95421 19.45106 galactic Aur Second-epoch detections are separated by 4.3" 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 | 07:01:14.06 +41:55:54.3 (user input) | T | P | (position from user input) SpType: DA 2015MNRAS.454.2787G LAMOST J070113.45+415554.6
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3222 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:14.06 +41:55:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3222 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:14.35 +42:06:00.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.52 06:58:35.98 +41:19:17.8
175.38614 18.78165 galactic Aur Second-epoch detections are separated by 0.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.6528+41.3220 | 06:58:35.98 +41:19:17.8 (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 J104.6528+41.3220,2461118.8222,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6528+41.3220 20260319.3222 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:35.98 +41:19:17.8 ;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_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.66 06:59:08.79 +42:19:17.7
174.42771 19.21651 galactic Aur Second-epoch detections are separated by 3.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.7951+42.3212 | 06:59:08.79 +42:19:17.7 (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 J104.7951+42.3212,2461118.8222,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7951+42.3212 20260319.3222 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:08.79 +42:19:17.7 ;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_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.33 06:58:19.87 +42:35:51.5
174.09891 19.16761 galactic Aur 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 | target | 06:58:19.87 +42:35:51.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3222 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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:19.87 +42:35:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.17 06:57:32.50 +42:44:55.2
173.89667 19.08182 galactic Aur Second-epoch detections are separated by 0.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 951340994140632448 | 06:57:33.14 +42:44:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 951340994140632448,2461118.8222,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 951340994140632448 20260319.3222 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:57:32.50 +42:44:55.2 ;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_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.13 06:58:13.71 +41:43:43.1
174.95693 18.85544 galactic Aur Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 951184661627764224 | 06:58:12.99 +41:43:46.6 (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 951184661627764224,2461118.8222,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 951184661627764224 20260319.3222 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:13.71 +41:43:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.32 08:16:27.06 +40:19:20.8
180.59256 32.75356 galactic Lyn Second-epoch detections are separated by 0.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:16:27.06 +40:19:20.8 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.025 (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,2461118.8222,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3222 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:27.06 +40:19:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3222 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:03:09.32 +33:48:08.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_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-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3257 2461118.8257 13.89 08:23:00.29 +17:45:45.7
206.26196 27.95662 galactic Cnc Second-epoch detections are separated by 1.4" 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 | target | 08:23:00.29 +17:45:45.7 (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,2461118.8257,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3257 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:00.29 +17:45:45.7 ;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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3257 2461118.8257 13.53 08:23:41.11 +18:46:29.3
205.26126 28.47906 galactic Cnc Second-epoch detections are separated by 4.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 662449918876959872 | 08:23:39.57 +18:45:48.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 662449918876959872,2461118.8257,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 662449918876959872 20260319.3257 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:41.11 +18:46:29.3 ;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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3257 2461118.8257 13.52 08:23:13.02 +18:34:49.1
205.42122 28.30492 galactic Cnc Second-epoch detections are separated by 2.6" 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 | 08:23:13.02 +18:34:49.1 (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,2461118.8257,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3257 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:13.02 +18:34:49.1 ;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-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3257 2461118.8257 13.56 08:24:56.39 +18:57:21.0
205.19158 28.82130 galactic Cnc Second-epoch detections are separated by 2.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:24:56.39 +18:57:21.0 (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,2461118.8257,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3257 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2025-12-23_03-55-37_20.00sec_-14.90C_LIGHT_0522.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-05-Q2b1x1_025352_TTUQ2b1x1_31394_KemzguHo/fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20.00sec_-15.00C_LIGHT_0049.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:56.39 +18:57:21.0 ;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_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-49-12_20_00sec_-15_00C_LIGHT_0049_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2025-12-23_03-55-37_20_00sec_-14_90C_LIGHT_0522_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-19_02-48-22_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 11.12 07:33:11.73 +18:24:45.0
200.67492 17.27939 galactic Gem Second-epoch detections are separated by 1.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3170221743224396544 | 07:33:10.41 +18:25:06.9 (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 3170221743224396544,2461118.8111,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3170221743224396544 20260319.3111 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:11.73 +18:24:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-59_20_00sec_-15_00C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-59_20_00sec_-15_00C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-59_20_00sec_-15_00C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-59_20_00sec_-15_00C_LIGHT_0479_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8111,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3111 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:31:23.47 +09:17:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 13.99 07:33:31.28 +18:15:49.2
200.85017 17.29074 galactic Gem Second-epoch detections are separated by 7.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J113.3887+18.2737 | 07:33:31.28 +18:15:49.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J113.3887+18.2737,2461118.8111,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J113.3887+18.2737 20260319.3111 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:31.28 +18:15:49.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 14.04 07:28:58.16 +18:52:48.8
199.80798 16.54934 galactic Gem Second-epoch detections are separated by 2.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:28:58.16 +18:52:48.8 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8111,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3111 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:28:58.16 +18:52:48.8 ;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_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8111,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3111 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:31:16.70 +18:52:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8111,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3111 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:29:23.17 +18:22:08.7 ;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_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 13.26 07:30:53.86 +18:09:37.8
200.68745 16.67867 galactic Gem Second-epoch detections are separated by 2.9" 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 3170200951286506112 | 07:30:53.43 +18:09:39.5 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3170200951286506112,2461118.8111,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3170200951286506112 20260319.3111 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:30:53.86 +18:09:37.8 ;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_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 13.28 07:28:18.51 +18:14:06.5
200.35756 16.14617 galactic Gem Second-epoch detections are separated by 3.1" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3170309429277287168 | 07:28:19.04 +18:14:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3170309429277287168,2461118.8111,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3170309429277287168 20260319.3111 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:28:18.51 +18:14:06.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 13.13 07:30:51.10 +18:34:36.6
200.28471 16.83595 galactic Gem Second-epoch detections are separated by 7.2" 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 3170409416115799296 | 07:30:50.69 +18:34:42.6 (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 3170409416115799296,2461118.8111,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3170409416115799296 20260319.3111 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:30:51.10 +18:34:36.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 13.09 07:30:06.55 +18:54:09.8
199.89920 16.80539 galactic Gem Second-epoch detections are separated by 2.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3170499576069060608 | 07:30:07.01 +18:54:09.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3170499576069060608,2461118.8111,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3170499576069060608 20260319.3111 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:30:06.55 +18:54:09.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 13.02 07:28:53.59 +17:51:17.2
200.77818 16.11919 galactic Gem Second-epoch detections are separated by 3.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3170099040302740736 | 07:28:54.12 +17:51:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3170099040302740736,2461118.8111,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3170099040302740736 20260319.3111 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:28:53.59 +17:51:17.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 12.46 07:29:22.87 +09:09:16.7
208.97208 12.55353 galactic CMi Second-epoch detections are separated by 1.3" 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 3143483235345548928 | 07:29:21.85 +09:08:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3143483235345548928,2461118.8111,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3143483235345548928 20260319.3111 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:29:22.87 +09:09:16.7 ;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_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 12.51 07:28:32.91 +16:27:19.9
202.07046 15.47231 galactic Gem Second-epoch detections are separated by 2.3" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J112.1389+16.4551 | 07:28:33.35 +16:27:18.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J112.1389+16.4551,2461118.8111,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J112.1389+16.4551 20260319.3111 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 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:28:32.91 +16:27:19.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 12.41 07:29:51.63 +18:10:39.8
200.56740 16.46014 galactic Gem Second-epoch detections are separated by 1.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J112.4624+18.1779 | 07:29:50.98 +18:10:40.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J112.4624+18.1779,2461118.8111,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J112.4624+18.1779 20260319.3111 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 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:29:51.63 +18:10:39.8 ;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_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 12.62 08:30:08.58 +17:16:19.5
207.50316 29.35323 galactic Cnc Second-epoch detections are separated by 0.1" 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 | target | 08:30:08.58 +17:16:19.5 (user input) | T | P | (position from user input) SpType: A9V (LAMOST DR5) J-Ks=0.197+/-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
target,2461118.8111,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3111 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:08.58 +17:16:19.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 13.23 08:29:22.95 +17:05:02.3
207.62526 29.11442 galactic Cnc Second-epoch detections are separated by 0.5" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:29:22.95 +17:05:02.3 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.521+/-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,2461118.8111,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3111 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:22.95 +17:05:02.3 ;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_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 12.43 08:30:21.50 +18:19:27.4
206.40021 29.78857 galactic Cnc Second-epoch detections are separated by 0.7" 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 662233452525369600 | 08:30:21.54 +18:19:27.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.401+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 662233452525369600,2461118.8111,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 662233452525369600 20260319.3111 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 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:21.50 +18:19:27.4 ;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_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 11.87 07:32:15.36 +09:56:15.8
208.56550 13.53264 galactic CMi Second-epoch detections are separated by 1.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3149553432883856000 | 07:32:15.18 +09:56:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3149553432883856000,2461118.8111,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3149553432883856000 20260319.3111 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 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:32:15.36 +09:56:15.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3111 2461118.8111 12.52 08:30:06.01 +18:32:49.2
206.13544 29.81236 galactic Cnc Second-epoch detections are separated by 1.1" 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 | Gaia DR3 662288153228733312 | 08:30:05.96 +18:32:48.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.329+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 662288153228733312,2461118.8111,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 662288153228733312 20260319.3111 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 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-05_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q2b1x1_2025-12-23_03-15-59_20.00sec_-15.00C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20.00sec_-14.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-04-Q2b1x1_025145_TTUQ2b1x1_24749_bepXUAVB/fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20.00sec_-15.00C_LIGHT_0024.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:06.01 +18:32:49.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-28-13_20_00sec_-15_00C_LIGHT_0024_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-04-Q2b1x1_2025-12-23_03-15-05_20_00sec_-15_00C_LIGHT_0478_fits__*pix.png resample_wcs_fd_Cnc-04-Q2b1x1_2026-03-19_02-27-26_20_00sec_-14_90C_LIGHT_0023_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 14.12 08:05:19.72 +11:01:32.5
211.18480 21.34583 galactic Cnc Second-epoch detections are separated by 4.0" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:05:19.72 +11:01:32.5 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:19.72 +11:01:32.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 13.97 08:07:07.09 +09:46:10.7
212.60547 21.20876 galactic Cnc Second-epoch detections are separated by 4.0" and 1.7 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 | 08:07:07.09 +09:46:10.7 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:07:07.09 +09:46:10.7 ;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_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:36.00 +10:15:09.9 ;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_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 13.65 08:04:24.56 +07:44:15.6
214.24784 19.72235 galactic Cnc Second-epoch detections are separated by 2.2" and 2.1 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 | 08:04:24.56 +07:44:15.6 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:24.56 +07:44:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 12.94 08:04:18.14 +09:15:39.4
212.77648 20.36306 galactic Cnc Second-epoch detections are separated by 0.6" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3146302898555059968 | 08:04:18.58 +09:15:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3146302898555059968,2461118.8151,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3146302898555059968 20260319.3151 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:18.14 +09:15:39.4 ;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_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 12.60 08:04:41.77 +09:57:26.3
212.14981 20.75041 galactic Cnc Second-epoch detections are separated by 6.7" and 0.9 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 3147469171155327360 | 08:04:41.31 +09:57:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3147469171155327360,2461118.8151,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3147469171155327360 20260319.3151 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:04:41.77 +09:57:26.3 ;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_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 12.77 08:03:49.87 +01:34:29.3
219.96000 16.79213 galactic CMi Second-epoch detections are separated by 2.8" 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 | Gaia DR3 3084852327551323008 | 08:03:49.68 +01:34:30.2 (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 3084852327551323008,2461118.8151,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3084852327551323008 20260319.3151 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:49.87 +01:34:29.3 ;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_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3151 2461118.8151 13.08 09:01:52.71 +08:05:24.2
220.98839 32.61759 galactic Cnc Second-epoch detections are separated by 1.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:01:52.71 +08:05:24.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.574+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8151,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3151 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20.00sec_-14.90C_LIGHT_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-01-Q2b1x1_025549_TTUQ2b1x1_25181_Z3L1f3tp/fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20.00sec_-15.00C_LIGHT_0030.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:52.71 +08:05:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-56_20_00sec_-15_00C_LIGHT_0030_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-19_02-33-12_20_00sec_-14_90C_LIGHT_0029_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 14.10 07:46:26.44 +26:36:50.0
193.76873 23.16643 galactic Gem Second-epoch detections are separated by 3.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:46:26.44 +26:36:50.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8201,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3201 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:26.44 +26:36:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.98 07:51:14.48 +19:30:42.5
201.36569 21.63680 galactic Gem Second-epoch detections are separated by 1.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:51:14.48 +19:30:42.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8201,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3201 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:14.48 +19:30:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 14.06 07:46:33.53 +24:50:55.4
195.57621 22.58060 galactic Gem Second-epoch detections are separated by 2.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:46:33.53 +24:50:55.4 (user input) | T | P | (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
target,2461118.8201,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3201 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:33.53 +24:50:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8201,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3201 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:47:50.85 +26:38:28.2 ;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_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.62 07:45:57.50 +25:58:21.8
194.38285 22.84510 galactic Gem Second-epoch detections are separated by 2.8" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:45:57.50 +25:58:21.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8201,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3201 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:57.50 +25:58:21.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.50 08:33:34.76 +18:17:13.7
206.76138 30.48734 galactic Cnc Second-epoch detections are separated by 7.2" 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 659593353307603200 | 08:33:35.37 +18:17:07.8 (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 659593353307603200,2461118.8201,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 659593353307603200 20260319.3201 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:33:34.76 +18:17:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.63 07:46:14.11 +26:44:59.3
193.61272 23.16947 galactic Gem Second-epoch detections are separated by 0.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 874912085468209664 | 07:46:13.46 +26:45:06.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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
Gaia DR3 874912085468209664,2461118.8201,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 874912085468209664 20260319.3201 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:14.11 +26:44:59.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 13.15 07:45:12.65 +26:14:13.2
194.05096 22.77870 galactic Gem Second-epoch detections are separated by 4.0" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 868889304368489472 | 07:45:12.11 +26:14:17.2 (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 868889304368489472,2461118.8201,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 868889304368489472 20260319.3201 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:12.65 +26:14:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3201 2461118.8201 12.59 08:52:33.10 +26:10:11.7
199.42493 37.14536 galactic Cnc Second-epoch detections are separated by 0.6" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:52:33.10 +26:10:11.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8201,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3201 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 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20.00sec_-14.90C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-02-Q2b1x1_024945_TTUQ2b1x1_14109_Ut0ka7D2/fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20.00sec_-15.00C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:52:33.10 +26:10:11.7 ;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_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-41-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q2b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q2b1x1_2026-03-19_02-40-20_20_00sec_-14_90C_LIGHT_0038_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3234 2461118.8234 13.42 08:57:51.45 +01:42:27.8
226.93697 28.67153 galactic Hya Second-epoch detections are separated by 2.7" 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 | target | 08:57:51.45 +01:42:27.8 (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,2461118.8234,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3234 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:51.45 +01:42:27.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20_00sec_-15_00C_LIGHT_0045_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8268,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3268 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:40.20 +10:24:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8268,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3268 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:56:01.69 +10:45:33.0 ;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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3268 2461118.8268 13.66 08:55:32.59 +10:05:23.9
218.04380 32.10815 galactic Cnc Second-epoch detections are separated by 2.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:55:32.59 +10:05:23.9 (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,2461118.8268,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3268 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:32.59 +10:05:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3268 2461118.8268 13.41 08:55:11.77 +10:18:50.6
217.76169 32.12850 galactic Cnc Second-epoch detections are separated by 4.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 597773307740039936 | 08:55:12.42 +10:18:48.3 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 597773307740039936,2461118.8268,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 597773307740039936 20260319.3268 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:11.77 +10:18:50.6 ;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_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3268 2461118.8268 13.23 08:55:49.24 +02:02:39.2
226.31506 28.39998 galactic Hya Second-epoch detections are separated by 5.0" 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 | target | 08:55:49.24 +02:02:39.2 (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,2461118.8268,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3268 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:49.24 +02:02:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3268* 09 53 40.99 +01 34 45.6 13.6 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8268,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3268 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-02-Q2b1x1_025754_TTUQ2b1x1_3892_YPuTihbN/fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20.00sec_-15.00C_LIGHT_0051.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:53:40.99 +01:34:45.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-50-46_20_00sec_-15_00C_LIGHT_0051_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-19_02-49-58_20_00sec_-14_90C_LIGHT_0050_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3190* 09 48 00.17 -04 50 11.2 13.9 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8190,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3190 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-03-Q2b1x1_2025-12-23_03-51-09_20.00sec_-14.90C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-03-Q2b1x1_030146_TTUQ2b1x1_5557_zphigPfq/fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-03-Q2b1x1_030146_TTUQ2b1x1_5557_zphigPfq/fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20.00sec_-15.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:48:00.17 -04:50:11.2 ;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_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20_00sec_-15_00C_LIGHT_0037_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20_00sec_-14_90C_LIGHT_0036_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-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20_00sec_-15_00C_LIGHT_0037_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20_00sec_-14_90C_LIGHT_0036_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3190 2461118.8190 13.85 09:49:01.78 -05:22:32.3
242.34235 35.25467 galactic Sex Second-epoch detections are separated by 3.6" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:49:01.78 -05:22:32.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3190* 09 49 01.78 -05 22 32.3 13.8 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8190,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3190 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-03-Q2b1x1_2025-12-23_03-51-09_20.00sec_-14.90C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-03-Q2b1x1_030146_TTUQ2b1x1_5557_zphigPfq/fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-03-Q2b1x1_030146_TTUQ2b1x1_5557_zphigPfq/fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20.00sec_-15.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:49:01.78 -05:22:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20_00sec_-15_00C_LIGHT_0037_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20_00sec_-14_90C_LIGHT_0036_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-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20_00sec_-15_00C_LIGHT_0037_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20_00sec_-14_90C_LIGHT_0036_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3190* 09 49 06.01 -05 10 00.8 13.5 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8190,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3190 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-03-Q2b1x1_2025-12-23_03-51-09_20.00sec_-14.90C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-03-Q2b1x1_030146_TTUQ2b1x1_5557_zphigPfq/fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-03-Q2b1x1_030146_TTUQ2b1x1_5557_zphigPfq/fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20.00sec_-15.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:49:06.01 -05:10:00.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20_00sec_-15_00C_LIGHT_0037_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20_00sec_-14_90C_LIGHT_0036_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-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20_00sec_-15_00C_LIGHT_0037_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20_00sec_-14_90C_LIGHT_0036_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3190 2461118.8190 12.81 09:47:29.81 -05:59:43.8
242.63828 34.56856 galactic Sex Second-epoch detections are separated by 2.3" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3820963886191482496 | 09:47:29.34 -05:59:42.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3190* 09 47 29.81 -05 59 43.8 12.8 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3820963886191482496,2461118.8190,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3820963886191482496 20260319.3190 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-03-Q2b1x1_2025-12-23_03-51-09_20.00sec_-14.90C_LIGHT_0518.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-03-Q2b1x1_030146_TTUQ2b1x1_5557_zphigPfq/fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-03-Q2b1x1_030146_TTUQ2b1x1_5557_zphigPfq/fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20.00sec_-15.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:47:29.81 -05:59:43.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20_00sec_-15_00C_LIGHT_0037_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20_00sec_-14_90C_LIGHT_0036_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-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-39-31_20_00sec_-15_00C_LIGHT_0037_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-03-Q2b1x1_2025-12-23_03-51-09_20_00sec_-14_90C_LIGHT_0518_fits__*pix.png resample_wcs_fd_Sex-03-Q2b1x1_2026-03-19_02-38-46_20_00sec_-14_90C_LIGHT_0036_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3332 2461118.8332 14.40 11:34:23.25 -09:40:47.3
273.39686 48.72324 galactic Crt Second-epoch detections are separated by 2.5" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J173.5970-09.6800 | 11:34:23.25 -09:40:47.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.003+/-0.127 (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 J173.5970-09.6800,2461118.8332,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J173.5970-09.6800 20260319.3332 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-01-Q2b1x1_030345_TTUQ2b1x1_16578_f5nY1qH4/fd_Crt-01-Q2b1x1_2026-03-19_02-59-18_20.00sec_-14.90C_LIGHT_0060.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-01-Q2b1x1_030345_TTUQ2b1x1_16578_f5nY1qH4/fd_Crt-01-Q2b1x1_2026-03-19_03-00-04_20.00sec_-14.90C_LIGHT_0061.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:23.25 -09:40:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q2b1x1_2026-03-19_03-00-04_20_00sec_-14_90C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q2b1x1_2026-03-19_02-59-18_20_00sec_-14_90C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q2b1x1_2026-03-19_03-00-04_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q2b1x1_2026-03-19_02-59-18_20_00sec_-14_90C_LIGHT_0060_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3332 2461118.8332 14.39 11:38:03.58 -06:13:58.2
272.22925 52.20987 galactic Vir Second-epoch detections are separated by 5.2" 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 | target | 11:38:03.58 -06:13:58.2 (user input) | T | P | (position from user input) J-Ks=1.237+/-0.209 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3332* 11 38 03.58 -06 13 58.2 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8332,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3332 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q2b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-01-Q2b1x1_030345_TTUQ2b1x1_16578_f5nY1qH4/fd_Crt-01-Q2b1x1_2026-03-19_02-59-18_20.00sec_-14.90C_LIGHT_0060.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-01-Q2b1x1_030345_TTUQ2b1x1_16578_f5nY1qH4/fd_Crt-01-Q2b1x1_2026-03-19_03-00-04_20.00sec_-14.90C_LIGHT_0061.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:03.58 -06:13:58.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q2b1x1_2026-03-19_03-00-04_20_00sec_-14_90C_LIGHT_0061_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q2b1x1_2026-03-19_02-59-18_20_00sec_-14_90C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q2b1x1_2026-03-19_03-00-04_20_00sec_-14_90C_LIGHT_0061_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-01-Q2b1x1_2026-01-18_04-04-38_20_00sec_-14_90C_LIGHT_0477_fits__*pix.png resample_wcs_fd_Crt-01-Q2b1x1_2026-03-19_02-59-18_20_00sec_-14_90C_LIGHT_0060_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3179 2461118.8179 13.73 10:08:44.45 -14:01:52.0
254.01585 32.97681 galactic Hya Second-epoch detections are separated by 1.2" 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 J152.1833-14.0307 | 10:08:44.45 -14:01:52.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J152.1833-14.0307,2461118.8179,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J152.1833-14.0307 20260319.3179 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_030800_TTUQ2b1x1_18829_hpZcbKjo/fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_030800_TTUQ2b1x1_18829_hpZcbKjo/fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20.00sec_-15.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:08:44.45 -14:01:52.0 ;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_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20_00sec_-15_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20_00sec_-15_00C_LIGHT_0034_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-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20_00sec_-15_00C_LIGHT_0034_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8179,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3179 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_030800_TTUQ2b1x1_18829_hpZcbKjo/fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_030800_TTUQ2b1x1_18829_hpZcbKjo/fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20.00sec_-15.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:10:35.10 -13:13:44.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20_00sec_-15_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20_00sec_-15_00C_LIGHT_0034_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-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20_00sec_-15_00C_LIGHT_0034_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8179,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3179 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_030800_TTUQ2b1x1_18829_hpZcbKjo/fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_030800_TTUQ2b1x1_18829_hpZcbKjo/fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20.00sec_-15.00C_LIGHT_0035.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:08:54.99 -14:22:39.8 ;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_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20_00sec_-15_00C_LIGHT_0035_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20_00sec_-15_00C_LIGHT_0034_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-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-38-00_20_00sec_-15_00C_LIGHT_0035_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_02-37-12_20_00sec_-15_00C_LIGHT_0034_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3343 2461118.8343 9.84 11:15:19.74 -18:08:59.3
273.03652 39.07876 galactic Crt Second-epoch detections are separated by 0.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3558078971047964800 | 11:15:20.90 -18:08:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0V 1943ApJ....97..381V BD-17 3336
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3558078971047964800,2461118.8343,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3558078971047964800 20260319.3343 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_030956_TTUQ2b1x1_27937_K83AIeno/fd_Crt-02-Q2b1x1_2026-03-19_03-00-50_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_030956_TTUQ2b1x1_27937_K83AIeno/fd_Crt-02-Q2b1x1_2026-03-19_03-01-36_20.00sec_-14.90C_LIGHT_0063.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:15:19.74 -18:08:59.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_03-01-36_20_00sec_-14_90C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_03-00-50_20_00sec_-15_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_03-01-36_20_00sec_-14_90C_LIGHT_0063_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_03-00-50_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8343,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3343 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_030956_TTUQ2b1x1_27937_K83AIeno/fd_Crt-02-Q2b1x1_2026-03-19_03-00-50_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_030956_TTUQ2b1x1_27937_K83AIeno/fd_Crt-02-Q2b1x1_2026-03-19_03-01-36_20.00sec_-14.90C_LIGHT_0063.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:53:05.25 -18:22:39.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_03-01-36_20_00sec_-14_90C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_03-00-50_20_00sec_-15_00C_LIGHT_0062_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_03-01-36_20_00sec_-14_90C_LIGHT_0063_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_03-00-50_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8390,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3390 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 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-01-18_06-03-32_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Oph-07-Q2b1x1_031153_TTUQ2b1x1_20085_AUpnrVzi/fd_Oph-07-Q2b1x1_2026-03-19_03-07-30_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Oph-07-Q2b1x1_031153_TTUQ2b1x1_20085_AUpnrVzi/fd_Oph-07-Q2b1x1_2026-03-19_03-08-33_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:54:24.14 -22:44:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-19_03-08-33_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-19_03-07-30_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-19_03-08-33_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-19_03-07-30_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3390 2461118.8390 12.22 16:23:03.39 -21:48:29.2
354.57855 19.20666 galactic Sco Second-epoch detections are separated by 1.0" 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 | Gaia DR3 6052061884497420288 | 16:23:03.63 -21:48:26.6 (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 6052061884497420288,2461118.8390,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6052061884497420288 20260319.3390 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 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-01-18_06-03-32_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-01-21_05-51-26_20.00sec_-15.00C_LIGHT_0582.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Oph-07-Q2b1x1_031153_TTUQ2b1x1_20085_AUpnrVzi/fd_Oph-07-Q2b1x1_2026-03-19_03-07-30_20.00sec_-15.00C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Oph-07-Q2b1x1_031153_TTUQ2b1x1_20085_AUpnrVzi/fd_Oph-07-Q2b1x1_2026-03-19_03-08-33_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:23:03.39 -21:48:29.2 ;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_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-19_03-08-33_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-19_03-07-30_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-19_03-08-33_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-19_03-07-30_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8318,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3318 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:50:18.37 -29:34:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_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_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3318 2461118.8318 13.79 13:48:11.07 -30:27:06.4
317.17765 30.84536 galactic Cen Second-epoch detections are separated by 0.7" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6175067346967554688 | 13:48:11.07 -30:27:06.4 (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+/-0.093 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6175067346967554688,2461118.8318,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6175067346967554688 20260319.3318 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:48:11.07 -30:27:06.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_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_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3318 2461118.8318 13.71 13:16:20.28 -28:17:08.1
309.56663 34.26518 galactic Hya Second-epoch detections are separated by 1.9" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6183280458307235712 | 13:16:20.28 -28:17:08.1 (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=1.488+/-0.122 (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
Large-amplitude variable Gaia DR2 6183280458307235712,2461118.8318,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6183280458307235712 20260319.3318 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:16:20.28 -28:17:08.1 ;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-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_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_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3318 2461118.8318 13.93 13:24:53.45 -30:20:02.4
311.44317 31.98428 galactic Cen Second-epoch detections are separated by 2.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J201.2112-30.3304 | 13:24:53.45 -30:20:02.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.588+/-0.148 (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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J201.2112-30.3304,2461118.8318,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J201.2112-30.3304 20260319.3318 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 /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:24:53.45 -30:20:02.4 ;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_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_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_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_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,2461118.8318,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3318 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-13-Q2b1x1_2026-01-18_04-25-38_20.00sec_-15.00C_LIGHT_0501.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-13-Q2b1x1_031403_TTUQ2b1x1_17307_gjOiD9Ck/fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20.00sec_-15.00C_LIGHT_0059.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:59:57.25 -26:51:50.1 ;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_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_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_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-58_20_00sec_-15_00C_LIGHT_0059_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-13-Q2b1x1_2026-01-18_04-25-38_20_00sec_-15_00C_LIGHT_0501_fits__*pix.png resample_wcs_fd_Hya-13-Q2b1x1_2026-03-19_02-57-12_20_00sec_-15_00C_LIGHT_0058_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3306 2461118.8306 12.60 14:11:45.17 -37:04:56.2
320.25134 23.07357 galactic Cen Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117945102267619200 | 14:11:48.22 -37:04:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117945102267619200,2461118.8306,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6117945102267619200 20260319.3306 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q2b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20.00sec_-14.90C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:11:45.17 -37:04:56.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3306 2461118.8306 12.66 14:08:08.85 -38:26:21.5
319.04567 22.02031 galactic Cen Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117364392633794176 | 14:08:09.49 -38:26:21.8 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117364392633794176,2461118.8306,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6117364392633794176 20260319.3306 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q2b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20.00sec_-14.90C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:08.85 -38:26:21.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3306 2461118.8306 13.38 14:10:49.45 -37:22:29.8
319.95692 22.85830 galactic Cen Second-epoch detections are separated by 1.9" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:10:49.45 -37:22:29.8 (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,2461118.8306,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3306 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q2b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20.00sec_-14.90C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:49.45 -37:22:29.8 ;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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3306 2461118.8306 13.31 13:59:49.65 -37:08:47.7
317.76595 23.74731 galactic Cen Second-epoch detections are separated by 2.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:59:49.65 -37:08:47.7 (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,2461118.8306,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3306 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q2b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20.00sec_-14.90C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:59:49.65 -37:08:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3306 2461118.8306 13.50 14:08:49.45 -38:52:03.6
319.03477 21.57216 galactic Cen Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6117152045146310144 | 14:08:49.95 -38:52:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6117152045146310144,2461118.8306,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6117152045146310144 20260319.3306 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q2b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20.00sec_-14.90C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:08:49.45 -38:52:03.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3306 2461118.8306 13.48 14:09:29.11 -36:55:20.9
319.84296 23.37302 galactic Cen Second-epoch detections are separated by 1.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:09:29.11 -36:55:20.9 (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,2461118.8306,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3306 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q2b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20.00sec_-14.90C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:09:29.11 -36:55:20.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3306 2461118.8306 13.40 13:58:35.23 -37:31:06.9
317.39299 23.46030 galactic Cen Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:58:35.23 -37:31:06.9 (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,2461118.8306,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3306 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q2b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20.00sec_-14.90C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:58:35.23 -37:31:06.9 ;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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3306 2461118.8306 13.50 12:58:14.23 -35:47:30.5
304.48016 27.05950 galactic Cen Second-epoch detections are separated by 4.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:14.23 -35:47:30.5 (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,2461118.8306,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3306 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cen-02-Q2b1x1_2026-01-18_04-31-42_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cen-02-Q2b1x1_031557_TTUQ2b1x1_15398_m1JMFLFw/fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20.00sec_-14.90C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:58:14.23 -35:47:30.5 ;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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_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_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-56-13_20_00sec_-14_90C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cen-02-Q2b1x1_2026-01-18_04-31-42_20_00sec_-15_00C_LIGHT_0507_fits__*pix.png resample_wcs_fd_Cen-02-Q2b1x1_2026-03-19_02-55-26_20_00sec_-15_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8279,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3279 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:25.23 +56:57:54.4 ;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_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 13.38 06:10:41.15 +58:18:48.4
155.81420 17.77765 galactic Cam Second-epoch detections are separated by 8.0" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J092.6740+58.3092 | 06:10:41.15 +58:18:48.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.6740+58.3092,2461118.8279,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.6740+58.3092 20260319.3279 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:41.15 +58:18:48.4 ;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_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8279,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3279 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:01.44 +57:48:21.0 ;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_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8279,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3279 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:02.37 +56:34:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 13.44 06:07:14.34 +57:20:54.7
156.54870 16.97134 galactic Cam Second-epoch detections are separated by 2.7" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:07:14.34 +57:20:54.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8279,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3279 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:14.34 +57:20:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 13.45 06:09:52.01 +57:21:51.7
156.68309 17.30200 galactic Cam Second-epoch detections are separated by 4.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:09:52.01 +57:21:51.7 (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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8279,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3279 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:52.01 +57:21:51.7 ;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_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 13.28 06:13:12.49 +57:38:03.7
156.60790 17.82086 galactic Cam Second-epoch detections are separated by 1.2" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:13:12.49 +57:38:03.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8279,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3279 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:13:12.49 +57:38:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 12.57 06:09:43.30 +57:57:59.7
156.09599 17.52389 galactic Cam Second-epoch detections are separated by 4.8" 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 998949405243439488 | 06:09:44.14 +57:57:59.2 (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 998949405243439488,2461118.8279,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 998949405243439488 20260319.3279 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:43.30 +57:57:59.7 ;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_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8279,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3279 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:05.39 +54:43:49.0 ;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_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 12.60 06:16:28.92 +49:34:48.5
164.50571 15.03879 galactic Aur Second-epoch detections are separated by 0.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 970886982284495744 | 06:16:28.78 +49:34:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.702+/-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 970886982284495744,2461118.8279,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 970886982284495744 20260319.3279 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-30-16_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:28.92 +49:34:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 12.69 07:58:25.24 +57:47:27.0
159.70285 31.49943 galactic Lyn Second-epoch detections are separated by 0.9" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J119.5981+57.7924 | 07:58:25.24 +57:47:27.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.395+/-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 J119.5981+57.7924,2461118.8279,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J119.5981+57.7924 20260319.3279 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-30-16_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:58:25.24 +57:47:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 13.59 07:50:49.12 +57:47:17.3
159.65354 30.48732 galactic Lyn Second-epoch detections are separated by 2.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1082248608025365632 | 07:50:54.71 +57:47:17.9 (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 1082248608025365632,2461118.8279,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1082248608025365632 20260319.3279 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-30-16_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:49.12 +57:47:17.3 ;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-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 12.46 06:16:00.49 +49:44:33.6
164.31965 15.03610 galactic Aur Second-epoch detections are separated by 0.4" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 970890486977788800 | 06:16:00.28 +49:44:31.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 970890486977788800,2461118.8279,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 970890486977788800 20260319.3279 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-30-16_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:00.49 +49:44:33.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3279 2461118.8279 13.30 06:14:08.71 +51:27:17.7
162.57656 15.47332 galactic Aur Second-epoch detections are separated by 1.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:14:08.71 +51:27:17.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8279,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3279 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-29-08_20.00sec_-14.90C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-01-Q2b1x1_2025-12-23_03-30-16_20.00sec_-15.00C_LIGHT_0495.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-01-Q2b1x1_031800_TTUQ2b1x1_19931_tZBwKEJK/fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20.00sec_-15.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:08.71 +51:27:17.7 ;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_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-52-26_20_00sec_-15_00C_LIGHT_0053_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-01-Q2b1x1_2025-12-23_03-29-08_20_00sec_-14_90C_LIGHT_0494_fits__*pix.png resample_wcs_fd_Lyn-01-Q2b1x1_2026-03-19_02-51-38_20_00sec_-15_00C_LIGHT_0052_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8245,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3245 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:35.57 +49:28:22.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_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_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3245 2461118.8245 13.33 06:25:05.06 +49:36:58.0
165.05181 16.33018 galactic Aur Second-epoch detections are separated by 2.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:25:05.06 +49:36:58.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8245,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3245 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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:05.06 +49:36:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_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_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3245 2461118.8245 13.47 06:27:38.25 +49:49:11.0
165.02148 16.78944 galactic Aur Second-epoch detections are separated by 6.1" 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 | Gaia DR3 968090679400665216 | 06:27:38.78 +49:48:34.1 (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 968090679400665216,2461118.8245,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 968090679400665216 20260319.3245 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:38.25 +49:49:11.0 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_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_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3245 2461118.8245 13.49 06:25:52.57 +50:26:36.4
164.30682 16.76683 galactic Aur Second-epoch detections are separated by 3.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.4698+50.4415 | 06:25:52.57 +50:26:36.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.4698+50.4415,2461118.8245,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.4698+50.4415 20260319.3245 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:52.57 +50:26:36.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_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_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3245 2461118.8245 13.16 06:25:53.98 +50:24:22.8
164.34411 16.75607 galactic Aur Second-epoch detections are separated by 4.5" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 971131486182684800 | 06:25:53.06 +50:24:25.9 (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 971131486182684800,2461118.8245,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 971131486182684800 20260319.3245 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:53.98 +50:24:22.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_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_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3461 2461118.8461 13.86 07:41:02.41 +50:42:14.1
167.55561 28.28907 galactic Lyn Second-epoch detections are separated by 7.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J115.2731+50.7085 | 07:41:02.41 +50:42:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J115.2731+50.7085,2461118.8461,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J115.2731+50.7085 20260319.3461 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q2b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-04-Q2b1x1_032145_TTUQ2b1x1_29835_STcbv1dZ/fd_Lyn-04-Q2b1x1_2026-03-19_03-17-50_20.00sec_-14.90C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-04-Q2b1x1_032145_TTUQ2b1x1_29835_STcbv1dZ/fd_Lyn-04-Q2b1x1_2026-03-19_03-18-38_20.00sec_-15.00C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:02.41 +50:42:14.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-04-Q2b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q2b1x1_2026-03-19_03-18-38_20_00sec_-15_00C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-04-Q2b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q2b1x1_2026-03-19_03-17-50_20_00sec_-14_90C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q2b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q2b1x1_2026-03-19_03-18-38_20_00sec_-15_00C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q2b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q2b1x1_2026-03-19_03-17-50_20_00sec_-14_90C_LIGHT_0074_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3461 2461118.8461 13.48 07:36:25.07 +49:53:50.7
168.31188 27.42410 galactic Lyn Second-epoch detections are separated by 4.3" 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 | target | 07:36:25.07 +49:53:50.7 (user input) | T | P | (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
target,2461118.8461,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3461 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q2b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-04-Q2b1x1_032145_TTUQ2b1x1_29835_STcbv1dZ/fd_Lyn-04-Q2b1x1_2026-03-19_03-17-50_20.00sec_-14.90C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-04-Q2b1x1_032145_TTUQ2b1x1_29835_STcbv1dZ/fd_Lyn-04-Q2b1x1_2026-03-19_03-18-38_20.00sec_-15.00C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:36:25.07 +49:53:50.7 ;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_Lyn-04-Q2b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q2b1x1_2026-03-19_03-18-38_20_00sec_-15_00C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-04-Q2b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q2b1x1_2026-03-19_03-17-50_20_00sec_-14_90C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q2b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q2b1x1_2026-03-19_03-18-38_20_00sec_-15_00C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q2b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q2b1x1_2026-03-19_03-17-50_20_00sec_-14_90C_LIGHT_0074_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3376 2461118.8376 13.28 08:23:50.30 +33:31:34.2
188.86831 32.88356 galactic Lyn Second-epoch detections are separated by 2.4" and 1.5 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 | 08:23:50.30 +33:31:34.2 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8376,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3376 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-01-Q2b1x1_032543_TTUQ2b1x1_10639_FRPlvd0R/fd_Cnc-01-Q2b1x1_2026-03-19_03-05-34_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-01-Q2b1x1_032543_TTUQ2b1x1_10639_FRPlvd0R/fd_Cnc-01-Q2b1x1_2026-03-19_03-06-18_20.00sec_-14.90C_LIGHT_0069.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:23:50.30 +33:31:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-19_03-06-18_20_00sec_-14_90C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-19_03-05-34_20_00sec_-14_90C_LIGHT_0068_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-19_03-06-18_20_00sec_-14_90C_LIGHT_0069_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-19_03-05-34_20_00sec_-14_90C_LIGHT_0068_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8354,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3354 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cnc-03-Q2b1x1_032747_TTUQ2b1x1_10485_MipV0VYt/fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20.00sec_-15.00C_LIGHT_0065.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:41:04.89 +26:08:27.7 ;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_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20_00sec_-15_00C_LIGHT_0065_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20_00sec_-14_90C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-03-11_20_00sec_-15_00C_LIGHT_0065_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-19_03-02-26_20_00sec_-14_90C_LIGHT_0064_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3483 2461118.8483 13.76 09:15:34.82 +18:20:27.1
211.03445 39.82588 galactic Cnc Second-epoch detections are separated by 3.4" 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 | target | 09:15:34.82 +18:20:27.1 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8483,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3483 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:15:34.82 +18:20:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_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_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3483 2461118.8483 14.09 09:15:17.06 +18:32:41.7
210.75354 39.83103 galactic Cnc Second-epoch detections are separated by 3.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:17.06 +18:32:41.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8483,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3483 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:15:17.06 +18:32:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_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_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_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!
TCP 2026 03 19.3365* 09 49 09.24 -05 04 26.1 13.9 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8365,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3365 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-02-Q2b1x1_033343_TTUQ2b1x1_24580_fW1b162H/fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-02-Q2b1x1_033343_TTUQ2b1x1_24580_fW1b162H/fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:49:09.24 -05:04:26.1 ;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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20_00sec_-14_90C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20_00sec_-14_90C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3365 2461118.8365 14.00 09:49:24.47 +01:43:22.3
235.24758 39.57924 galactic Sex Second-epoch detections are separated by 1.3" 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 | 09:49:24.47 +01:43:22.3 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3365* 09 49 24.47 +01 43 22.3 14.0 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,2461118.8365,14.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3365 14.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-02-Q2b1x1_033343_TTUQ2b1x1_24580_fW1b162H/fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-02-Q2b1x1_033343_TTUQ2b1x1_24580_fW1b162H/fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:49:24.47 +01:43:22.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20_00sec_-14_90C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20_00sec_-14_90C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3365 2461118.8365 13.83 09:50:27.89 -01:26:05.5
238.73669 37.95369 galactic Sex Second-epoch detections are separated by 4.0" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:50:27.89 -01:26:05.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3365* 09 50 27.89 -01 26 05.5 13.8 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8365,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3365 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-02-Q2b1x1_033343_TTUQ2b1x1_24580_fW1b162H/fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sex-02-Q2b1x1_033343_TTUQ2b1x1_24580_fW1b162H/fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:50:27.89 -01:26:05.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20_00sec_-14_90C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-45_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-19_03-04-00_20_00sec_-14_90C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3533 2461118.8533 14.14 11:31:32.06 -02:18:32.7
266.59493 54.82460 galactic Leo Second-epoch detections are separated by 4.3" 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 J172.8835-02.3093 | 11:31:32.06 -02:18:32.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.054+/-0.158 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3533* 11 31 32.06 -02 18 32.7 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J172.8835-02.3093,2461118.8533,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J172.8835-02.3093 20260319.3533 14.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:31:32.06 -02:18:32.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_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_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_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,2461118.8508,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3508 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-07-Q2b1x1_2025-12-23_03-47-27_20.00sec_-14.90C_LIGHT_0514.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-07-Q2b1x1_033947_TTUQ2b1x1_3832_DIPbeAsC/fd_Cam-07-Q2b1x1_2026-03-19_03-24-36_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-07-Q2b1x1_033947_TTUQ2b1x1_3832_DIPbeAsC/fd_Cam-07-Q2b1x1_2026-03-19_03-25-29_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:23.82 +72:30:57.0 ;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_Cam-07-Q2b1x1_2025-12-23_03-47-27_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png resample_wcs_fd_Cam-07-Q2b1x1_2026-03-19_03-25-29_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-07-Q2b1x1_2025-12-23_03-47-27_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png resample_wcs_fd_Cam-07-Q2b1x1_2026-03-19_03-24-36_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-07-Q2b1x1_2025-12-23_03-47-27_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png resample_wcs_fd_Cam-07-Q2b1x1_2026-03-19_03-25-29_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-07-Q2b1x1_2025-12-23_03-47-27_20_00sec_-14_90C_LIGHT_0514_fits__*pix.png resample_wcs_fd_Cam-07-Q2b1x1_2026-03-19_03-24-36_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3579 2461118.8579 12.89 09:35:30.51 +64:21:11.7
148.82380 41.59550 galactic UMa Second-epoch detections are separated by 1.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:35:30.51 +64:21:11.7 (user input) | T | P | (position from user input) J-Ks=0.371+/-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 03 19.3579* 09 35 30.51 +64 21 11.7 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,2461118.8579,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3579 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q2b1x1_2025-12-23_04-26-38_20.00sec_-15.00C_LIGHT_0554.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q2b1x1_2025-12-23_04-27-26_20.00sec_-15.00C_LIGHT_0555.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-02-Q2b1x1_034148_TTUQ2b1x1_11207_9hSV4EVt/fd_UMa-02-Q2b1x1_2026-03-19_03-34-48_20.00sec_-15.00C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-02-Q2b1x1_034148_TTUQ2b1x1_11207_9hSV4EVt/fd_UMa-02-Q2b1x1_2026-03-19_03-35-36_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:35:30.51 +64:21:11.7 ;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_UMa-02-Q2b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q2b1x1_2026-03-19_03-35-36_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-02-Q2b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q2b1x1_2026-03-19_03-34-48_20_00sec_-15_00C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-02-Q2b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q2b1x1_2026-03-19_03-35-36_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-02-Q2b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q2b1x1_2026-03-19_03-34-48_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3579 2461118.8579 13.34 07:45:53.25 +57:11:44.2
160.28334 29.78495 galactic Lyn Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J116.4721+57.1957 | 07:45:53.25 +57:11:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.316+/-0.031 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J116.4721+57.1957,2461118.8579,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J116.4721+57.1957 20260319.3579 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q2b1x1_2025-12-23_04-26-38_20.00sec_-15.00C_LIGHT_0554.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q2b1x1_2025-12-23_04-27-26_20.00sec_-15.00C_LIGHT_0555.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-02-Q2b1x1_034148_TTUQ2b1x1_11207_9hSV4EVt/fd_UMa-02-Q2b1x1_2026-03-19_03-34-48_20.00sec_-15.00C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-02-Q2b1x1_034148_TTUQ2b1x1_11207_9hSV4EVt/fd_UMa-02-Q2b1x1_2026-03-19_03-35-36_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:53.25 +57:11:44.2 ;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_UMa-02-Q2b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q2b1x1_2026-03-19_03-35-36_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-02-Q2b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q2b1x1_2026-03-19_03-34-48_20_00sec_-15_00C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-02-Q2b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q2b1x1_2026-03-19_03-35-36_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-02-Q2b1x1_2025-12-23_04-26-38_20_00sec_-15_00C_LIGHT_0554_fits__*pix.png resample_wcs_fd_UMa-02-Q2b1x1_2026-03-19_03-34-48_20_00sec_-15_00C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3636* 08 49 17.39 +49 17 02.2 14.3 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
target,2461118.8636,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3636 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2025-12-23_05-03-39_20.00sec_-15.00C_LIGHT_0598.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-09-Q2b1x1_034545_TTUQ2b1x1_25737_B0CKnlJS/fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-09-Q2b1x1_034545_TTUQ2b1x1_25737_B0CKnlJS/fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:49:17.39 +49:17:02.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3636* 08 49 46.85 +48 43 21.4 14.0 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,2461118.8636,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3636 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2025-12-23_05-03-39_20.00sec_-15.00C_LIGHT_0598.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-09-Q2b1x1_034545_TTUQ2b1x1_25737_B0CKnlJS/fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-09-Q2b1x1_034545_TTUQ2b1x1_25737_B0CKnlJS/fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:49:46.85 +48:43:21.4 ;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_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3636* 08 48 40.69 +50 22 55.2 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,2461118.8636,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3636 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2025-12-23_05-03-39_20.00sec_-15.00C_LIGHT_0598.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-09-Q2b1x1_034545_TTUQ2b1x1_25737_B0CKnlJS/fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-09-Q2b1x1_034545_TTUQ2b1x1_25737_B0CKnlJS/fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:40.69 +50:22:55.2 ;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_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3636 2461118.8636 13.66 08:54:24.91 +50:25:32.6
168.46225 39.89051 galactic UMa Second-epoch detections are separated by 2.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:54:24.91 +50:25:32.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3636* 08 54 24.91 +50 25 32.6 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,2461118.8636,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3636 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2025-12-23_05-03-39_20.00sec_-15.00C_LIGHT_0598.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-09-Q2b1x1_034545_TTUQ2b1x1_25737_B0CKnlJS/fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20.00sec_-14.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-09-Q2b1x1_034545_TTUQ2b1x1_25737_B0CKnlJS/fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20.00sec_-15.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:54:24.91 +50:25:32.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20_00sec_-15_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20_00sec_-14_90C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-43-45_20_00sec_-15_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-09-Q2b1x1_2025-12-23_05-03-39_20_00sec_-15_00C_LIGHT_0598_fits__*pix.png resample_wcs_fd_UMa-09-Q2b1x1_2026-03-19_03-42-58_20_00sec_-14_90C_LIGHT_0104_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3521 2461118.8521 12.04 08:46:10.68 +53:26:03.1
164.73712 38.36946 galactic UMa Second-epoch detections are separated by 5.9" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:46:10.68 +53:26:03.1 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3521* 08 46 10.68 +53 26 03.1 12.0 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,2461118.8521,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3521 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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20.00sec_-15.00C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:46:10.68 +53:26:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_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-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3521* 09 11 31.92 +54 53 37.5 13.9 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,2461118.8521,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3521 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20.00sec_-15.00C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:31.92 +54:53:37.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_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-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3521* 09 01 46.44 +48 35 46.5 13.9 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,2461118.8521,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3521 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20.00sec_-15.00C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:46.44 +48:35:46.5 ;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_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_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-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3521* 09 03 29.38 +49 21 03.6 13.9 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,2461118.8521,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3521 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20.00sec_-15.00C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:29.38 +49:21:03.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_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-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3521* 09 00 24.77 +55 17 18.8 14.0 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,2461118.8521,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3521 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q2b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20.00sec_-15.00C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-02-Q2b1x1_034351_TTUQ2b1x1_18525_dUubD4Ib/fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:24.77 +55:17:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_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-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-27-16_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q2b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q2b1x1_2026-03-19_03-26-30_20_00sec_-15_00C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3544 2461118.8544 14.25 10:42:38.01 +23:57:08.4
211.90892 60.85120 galactic LMi 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 | 10:42:38.01 +23:57:08.4 (user input) | T | P | (position from user input) J-Ks=1.081+/-0.100 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8544,14.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3544 14.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-02-Q2b1x1_035144_TTUQ2b1x1_27829_AW90KM1Y/fd_Leo-02-Q2b1x1_2026-03-19_03-29-44_20.00sec_-14.90C_LIGHT_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-02-Q2b1x1_035144_TTUQ2b1x1_27829_AW90KM1Y/fd_Leo-02-Q2b1x1_2026-03-19_03-30-36_20.00sec_-14.90C_LIGHT_0089.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:42:38.01 +23:57:08.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-19_03-30-36_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-19_03-29-44_20_00sec_-14_90C_LIGHT_0088_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-19_03-30-36_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-19_03-29-44_20_00sec_-14_90C_LIGHT_0088_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3688 2461118.8688 10.76 13:45:01.78 -19:54:46.5
319.76292 41.20074 galactic Vir Second-epoch detections are separated by 0.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6292194712901373824 | 13:45:01.41 -19:55:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.412+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3688* 13 45 01.78 -19 54 46.5 10.8 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6292194712901373824,2461118.8688,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6292194712901373824 20260319.3688 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-11_04-10-55_20.00sec_-14.90C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-13-Q2b1x1_040953_TTUQ2b1x1_2906_lz4tfbZZ/fd_Vir-13-Q2b1x1_2026-03-19_03-50-30_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-13-Q2b1x1_040953_TTUQ2b1x1_2906_lz4tfbZZ/fd_Vir-13-Q2b1x1_2026-03-19_03-51-17_20.00sec_-14.90C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:45:01.78 -19:54:46.5 ;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_Vir-13-Q2b1x1_2026-02-11_04-10-55_20_00sec_-14_90C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-19_03-51-17_20_00sec_-14_90C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-13-Q2b1x1_2026-02-11_04-10-55_20_00sec_-14_90C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-19_03-50-30_20_00sec_-15_00C_LIGHT_0112_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-13-Q2b1x1_2026-02-11_04-10-55_20_00sec_-14_90C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-19_03-51-17_20_00sec_-14_90C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-13-Q2b1x1_2026-02-11_04-10-55_20_00sec_-14_90C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-19_03-50-30_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3688 2461118.8688 14.44 12:53:52.17 -18:51:47.0
303.73168 44.00492 galactic Crv Second-epoch detections are separated by 1.9" 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 J193.4680-18.8641 | 12:53:52.17 -18:51:47.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J193.4680-18.8641,2461118.8688,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J193.4680-18.8641 20260319.3688 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-11_04-10-55_20.00sec_-14.90C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-13-Q2b1x1_040953_TTUQ2b1x1_2906_lz4tfbZZ/fd_Vir-13-Q2b1x1_2026-03-19_03-50-30_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-13-Q2b1x1_040953_TTUQ2b1x1_2906_lz4tfbZZ/fd_Vir-13-Q2b1x1_2026-03-19_03-51-17_20.00sec_-14.90C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:53:52.17 -18:51:47.0 ;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_Vir-13-Q2b1x1_2026-02-11_04-10-55_20_00sec_-14_90C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-19_03-51-17_20_00sec_-14_90C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-13-Q2b1x1_2026-02-11_04-10-55_20_00sec_-14_90C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-19_03-50-30_20_00sec_-15_00C_LIGHT_0112_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-13-Q2b1x1_2026-02-11_04-10-55_20_00sec_-14_90C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-19_03-51-17_20_00sec_-14_90C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-13-Q2b1x1_2026-02-11_04-10-55_20_00sec_-14_90C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Vir-13-Q2b1x1_2026-03-19_03-50-30_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3649 2461118.8649 9.55 14:47:44.94 -27:58:56.8
332.08179 28.22488 galactic Hya Second-epoch detections are separated by 0.1" 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 6219414155609249792 | 14:47:45.06 -27:58:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.042+/-0.039 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6219414155609249792,2461118.8649,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6219414155609249792 20260319.3649 9.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-01-09_04-32-00_20.00sec_-14.90C_LIGHT_0095.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-01-09_04-32-37_20.00sec_-15.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-14-Q2b1x1_041149_TTUQ2b1x1_18261_gD04g07I/fd_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-14-Q2b1x1_041149_TTUQ2b1x1_18261_gD04g07I/fd_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:47:44.94 -27:58:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-14-Q2b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-03-19_03-45-42_20_00sec_-14_90C_LIGHT_0107_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-14-Q2b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-03-19_03-44-56_20_00sec_-15_00C_LIGHT_0106_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-14-Q2b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-03-19_03-45-42_20_00sec_-14_90C_LIGHT_0107_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-14-Q2b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-03-19_03-44-56_20_00sec_-15_00C_LIGHT_0106_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3700 2461118.8700 12.60 08:56:09.18 +58:11:23.1
158.44733 39.07685 galactic UMa Second-epoch detections are separated by 7.0" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1037610673616922368 | 08:56:08.43 +58:11:24.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3700* 08 56 09.18 +58 11 23.1 12.6 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 1037610673616922368,2461118.8700,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1037610673616922368 20260319.3700 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-06-Q2b1x1_2025-12-23_04-43-48_20.00sec_-15.00C_LIGHT_0574.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-06-Q2b1x1_041557_TTUQ2b1x1_13753_DUClgELs/fd_UMa-06-Q2b1x1_2026-03-19_03-52-14_20.00sec_-15.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-06-Q2b1x1_041557_TTUQ2b1x1_13753_DUClgELs/fd_UMa-06-Q2b1x1_2026-03-19_03-53-04_20.00sec_-14.90C_LIGHT_0115.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:56:09.18 +58:11:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-06-Q2b1x1_2025-12-23_04-43-48_20_00sec_-15_00C_LIGHT_0574_fits__*pix.png resample_wcs_fd_UMa-06-Q2b1x1_2026-03-19_03-53-04_20_00sec_-14_90C_LIGHT_0115_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-06-Q2b1x1_2025-12-23_04-43-48_20_00sec_-15_00C_LIGHT_0574_fits__*pix.png resample_wcs_fd_UMa-06-Q2b1x1_2026-03-19_03-52-14_20_00sec_-15_00C_LIGHT_0114_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_UMa-06-Q2b1x1_2025-12-23_04-43-48_20_00sec_-15_00C_LIGHT_0574_fits__*pix.png resample_wcs_fd_UMa-06-Q2b1x1_2026-03-19_03-53-04_20_00sec_-14_90C_LIGHT_0115_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-06-Q2b1x1_2025-12-23_04-43-48_20_00sec_-15_00C_LIGHT_0574_fits__*pix.png resample_wcs_fd_UMa-06-Q2b1x1_2026-03-19_03-52-14_20_00sec_-15_00C_LIGHT_0114_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3723 2461118.8723 14.24 11:11:24.68 +26:57:49.8
207.59026 67.76454 galactic Leo Second-epoch detections are separated by 2.2" and 0.7 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 J167.8551+26.9637 | 11:11:24.68 +26:57:49.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3723* 11 11 24.68 +26 57 49.8 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J167.8551+26.9637,2461118.8723,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J167.8551+26.9637 20260319.3723 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2025-12-23_06-05-01_20.00sec_-15.00C_LIGHT_0666.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_LMi-02-Q2b1x1_042353_TTUQ2b1x1_16331_v8WgVBxp/fd_LMi-02-Q2b1x1_2026-03-19_03-55-30_20.00sec_-14.90C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_LMi-02-Q2b1x1_042353_TTUQ2b1x1_16331_v8WgVBxp/fd_LMi-02-Q2b1x1_2026-03-19_03-56-14_20.00sec_-15.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:11:24.68 +26:57:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_LMi-02-Q2b1x1_2025-12-23_06-05-01_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png resample_wcs_fd_LMi-02-Q2b1x1_2026-03-19_03-56-14_20_00sec_-15_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_LMi-02-Q2b1x1_2025-12-23_06-05-01_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png resample_wcs_fd_LMi-02-Q2b1x1_2026-03-19_03-55-30_20_00sec_-14_90C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_LMi-02-Q2b1x1_2025-12-23_06-05-01_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png resample_wcs_fd_LMi-02-Q2b1x1_2026-03-19_03-56-14_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_LMi-02-Q2b1x1_2025-12-23_06-05-01_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png resample_wcs_fd_LMi-02-Q2b1x1_2026-03-19_03-55-30_20_00sec_-14_90C_LIGHT_0118_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3814* 12 40 12.62 -05 47 53.3 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8814,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3814 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-07-Q2b1x1_042956_TTUQ2b1x1_32417_7HYPr9FN/fd_Vir-07-Q2b1x1_2026-03-19_04-08-38_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-07-Q2b1x1_042956_TTUQ2b1x1_32417_7HYPr9FN/fd_Vir-07-Q2b1x1_2026-03-19_04-09-22_20.00sec_-15.00C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:40:12.62 -05:47:53.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-19_04-09-22_20_00sec_-15_00C_LIGHT_0134_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-19_04-08-38_20_00sec_-14_90C_LIGHT_0133_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-19_04-09-22_20_00sec_-15_00C_LIGHT_0134_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-19_04-08-38_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3814* 12 51 13.24 -06 33 34.0 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8814,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3814 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-07-Q2b1x1_042956_TTUQ2b1x1_32417_7HYPr9FN/fd_Vir-07-Q2b1x1_2026-03-19_04-08-38_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-07-Q2b1x1_042956_TTUQ2b1x1_32417_7HYPr9FN/fd_Vir-07-Q2b1x1_2026-03-19_04-09-22_20.00sec_-15.00C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:51:13.24 -06:33:34.0 ;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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-19_04-09-22_20_00sec_-15_00C_LIGHT_0134_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-19_04-08-38_20_00sec_-14_90C_LIGHT_0133_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-19_04-09-22_20_00sec_-15_00C_LIGHT_0134_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-19_04-08-38_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8930,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3930 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-02-11_04-12-41_20.00sec_-14.90C_LIGHT_0484.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-14-Q2b1x1_043354_TTUQ2b1x1_17506_niyAARLC/fd_Vir-14-Q2b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-14-Q2b1x1_043354_TTUQ2b1x1_17506_niyAARLC/fd_Vir-14-Q2b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:27:13.45 -22:29:27.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-14-Q2b1x1_2026-02-11_04-12-41_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png resample_wcs_fd_Vir-14-Q2b1x1_2026-03-19_04-26-07_20_00sec_-14_90C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-14-Q2b1x1_2026-02-11_04-12-41_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png resample_wcs_fd_Vir-14-Q2b1x1_2026-03-19_04-25-20_20_00sec_-14_90C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-14-Q2b1x1_2026-02-11_04-12-41_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png resample_wcs_fd_Vir-14-Q2b1x1_2026-03-19_04-26-07_20_00sec_-14_90C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-14-Q2b1x1_2026-02-11_04-12-41_20_00sec_-14_90C_LIGHT_0484_fits__*pix.png resample_wcs_fd_Vir-14-Q2b1x1_2026-03-19_04-25-20_20_00sec_-14_90C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 14.29 19:50:56.19 +49:01:42.0
82.68753 11.21448 galactic Cyg 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 | target | 19:50:56.19 +49:01:42.0 (user input) | T | P | (position from user input) SpType: F8III/IV 2016AJ....151...13G LAMOST J195054.22+490134.3
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8997,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3997 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:56.19 +49:01:42.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8997,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3997 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:39.24 +41:44:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 13.62 21:04:48.55 +41:53:19.1
84.39506 -3.42335 galactic Cyg Second-epoch detections are separated by 1.3" 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 | ATO J316.1928+41.8898 | 21:04:47.83 +41:53:20.5 (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 J316.1928+41.8898,2461118.8997,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J316.1928+41.8898 20260319.3997 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:04:48.55 +41:53:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 13.34 21:00:53.74 +45:22:38.4
86.53689 -0.57889 galactic Cyg Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | NSV 13462 | 21:00:56.26 +45:22:55.2 (Gaia DR3) | SR (local) | 2458434.13300 (local) | Gaia3var=VARIABLE SpType: M7e 1973A&AS....9..183W UHA 108
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 13462,2461118.8997,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 13462 20260319.3997 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:00:53.74 +45:22:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 13.66 20:46:51.58 +43:56:04.3
83.82738 0.40531 galactic Cyg Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.7136+43.9361 | 20:46:51.58 +43:56:04.3 (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 J311.7136+43.9361,2461118.8997,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.7136+43.9361 20260319.3997 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:46:51.58 +43:56:04.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 13.79 20:53:26.71 +46:24:49.4
86.48048 1.07976 galactic Cyg 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 | ATO J313.3747+46.4110 | 20:53:28.16 +46:24:22.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J313.3747+46.4110,2461118.8997,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J313.3747+46.4110 20260319.3997 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:53:26.71 +46:24:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 13.80 20:28:48.10 +48:48:00.8
85.82898 5.82378 galactic Cyg Second-epoch detections are separated by 3.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J307.2187+48.7960 | 20:28:52.36 +48:48:19.9 (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 J307.2187+48.7960,2461118.8997,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J307.2187+48.7960 20260319.3997 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:28:48.10 +48:48:00.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 13.89 20:46:49.44 +49:56:07.0
88.51042 4.16310 galactic Cyg Second-epoch detections are separated by 2.3" 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 | Gaia DR3 2168346232608915072 | 20:46:50.28 +49:55:35.3 (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 2168346232608915072,2461118.8997,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168346232608915072 20260319.3997 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:46:49.44 +49:56:07.0 ;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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 13.88 20:39:50.91 +47:07:21.0
85.57730 3.33977 galactic Cyg Second-epoch detections are separated by 3.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J309.9615+47.1242 | 20:39:50.91 +47:07:21.0 (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 J309.9615+47.1242,2461118.8997,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J309.9615+47.1242 20260319.3997 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:39:50.91 +47:07:21.0 ;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_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3997 2461118.8997 14.23 20:40:35.99 +46:27:38.0
85.13028 2.83433 galactic Cyg Second-epoch detections are separated by 8.2" 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 J310.1778+46.4561 | 20:40:40.29 +46:27:30.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: em 1976VatOP...1..225W VES 274
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.1778+46.4561,2461118.8997,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J310.1778+46.4561 20260319.3997 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-03-Q2b1x1_2025-12-26_19-01-16_20.00sec_-15.00C_LIGHT_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-03-Q2b1x1_044146_TTUQ2b1x1_16086_Y0rOVOaB/fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:40:35.99 +46:27:38.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-53_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-03-Q2b1x1_2025-12-26_19-01-16_20_00sec_-15_00C_LIGHT_0002_fits__*pix.png resample_wcs_fd_Cyg-03-Q2b1x1_2026-03-19_04-35-00_20_00sec_-15_00C_LIGHT_0152_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4047 2461118.9047 14.21 13:49:46.70 -12:34:30.7
324.41529 47.84816 galactic Vir Second-epoch detections are separated by 1.8" 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 J207.4350-12.5684 | 13:49:46.70 -12:34:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4047* 13 49 46.70 -12 34 30.7 14.2 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J207.4350-12.5684,2461118.9047,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J207.4350-12.5684 20260319.4047 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:49:46.70 -12:34:30.7 ;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_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3970 2461118.8970 11.18 19:50:32.92 +18:05:55.9
55.76836 -4.25076 galactic Sge 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 | ATO J297.6392+18.0892 | 19:50:33.38 +18:05:54.9 (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 J297.6392+18.0892,2461118.8970,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.6392+18.0892 20260319.3970 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 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-01-18_06-34-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vul-01-Q2b1x1_044349_TTUQ2b1x1_18034_E9JMTfpr/fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20.00sec_-14.90C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vul-01-Q2b1x1_044349_TTUQ2b1x1_18034_E9JMTfpr/fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20.00sec_-14.90C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:32.92 +18:05:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20_00sec_-14_90C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20_00sec_-14_90C_LIGHT_0150_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20_00sec_-14_90C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20_00sec_-14_90C_LIGHT_0150_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3970 2461118.8970 11.41 19:49:01.02 +16:53:41.9
54.54080 -4.54176 galactic Sge Second-epoch detections are separated by 0.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1820801739657984640 | 19:49:01.51 +16:53:39.7 (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 1820801739657984640,2461118.8970,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1820801739657984640 20260319.3970 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-01-18_06-34-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vul-01-Q2b1x1_044349_TTUQ2b1x1_18034_E9JMTfpr/fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20.00sec_-14.90C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vul-01-Q2b1x1_044349_TTUQ2b1x1_18034_E9JMTfpr/fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20.00sec_-14.90C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:01.02 +16:53:41.9 ;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_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20_00sec_-14_90C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20_00sec_-14_90C_LIGHT_0150_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20_00sec_-14_90C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20_00sec_-14_90C_LIGHT_0150_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3970 2461118.8970 11.62 19:54:06.68 +17:01:43.0
55.27468 -5.52533 galactic Sge Second-epoch detections are separated by 5.1" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1820396191654942976 | 19:54:07.12 +17:01:40.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1820396191654942976,2461118.8970,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1820396191654942976 20260319.3970 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-01-18_06-34-53_20.00sec_-14.90C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vul-01-Q2b1x1_044349_TTUQ2b1x1_18034_E9JMTfpr/fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20.00sec_-14.90C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vul-01-Q2b1x1_044349_TTUQ2b1x1_18034_E9JMTfpr/fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20.00sec_-14.90C_LIGHT_0151.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:54:06.68 +17:01:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20_00sec_-14_90C_LIGHT_0151_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20_00sec_-14_90C_LIGHT_0150_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-34-11_20_00sec_-14_90C_LIGHT_0151_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-01-18_06-34-53_20_00sec_-14_90C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-19_04-28-52_20_00sec_-14_90C_LIGHT_0150_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4020 2461118.9020 11.04 18:29:57.13 -15:00:14.9
17.15871 -2.15345 galactic Sct Second-epoch detections are separated by 0.9" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4103957215445682432 | 18:29:57.70 -15:00:20.4 (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 4103957215445682432,2461118.9020,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4103957215445682432 20260319.4020 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-01-18_06-39-24_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Oph-06-Q2b1x1_045359_TTUQ2b1x1_2847_sn4jVvo4/fd_Oph-06-Q2b1x1_2026-03-19_04-38-16_20.00sec_-14.90C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Oph-06-Q2b1x1_045359_TTUQ2b1x1_2847_sn4jVvo4/fd_Oph-06-Q2b1x1_2026-03-19_04-39-05_20.00sec_-15.00C_LIGHT_0157.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:29:57.13 -15:00:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-19_04-39-05_20_00sec_-15_00C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-19_04-38-16_20_00sec_-14_90C_LIGHT_0156_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-19_04-39-05_20_00sec_-15_00C_LIGHT_0157_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-19_04-38-16_20_00sec_-14_90C_LIGHT_0156_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4020 2461118.9020 11.09 18:30:47.00 -15:06:35.0
17.15775 -2.38019 galactic Sct Second-epoch detections are separated by 0.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4103951924045609856 | 18:30:47.42 -15:06:39.2 (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 4103951924045609856,2461118.9020,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4103951924045609856 20260319.4020 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-01-18_06-39-24_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Oph-06-Q2b1x1_045359_TTUQ2b1x1_2847_sn4jVvo4/fd_Oph-06-Q2b1x1_2026-03-19_04-38-16_20.00sec_-14.90C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Oph-06-Q2b1x1_045359_TTUQ2b1x1_2847_sn4jVvo4/fd_Oph-06-Q2b1x1_2026-03-19_04-39-05_20.00sec_-15.00C_LIGHT_0157.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:30:47.00 -15:06:35.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-19_04-39-05_20_00sec_-15_00C_LIGHT_0157_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-19_04-38-16_20_00sec_-14_90C_LIGHT_0156_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-19_04-39-05_20_00sec_-15_00C_LIGHT_0157_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-03-19_04-38-16_20_00sec_-14_90C_LIGHT_0156_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4031 2461118.9031 10.10 16:54:42.49 -30:14:36.9
352.60110 8.34992 galactic Sco Second-epoch detections are separated by 1.2" 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 6029500597440292352 | 16:54:42.98 -30:14:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6029500597440292352,2461118.9031,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6029500597440292352 20260319.4031 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sco-02-Q2b1x1_045556_TTUQ2b1x1_22913_HE200OHy/fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sco-02-Q2b1x1_045556_TTUQ2b1x1_22913_HE200OHy/fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20.00sec_-15.00C_LIGHT_0159.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:54:42.49 -30:14:36.9 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20_00sec_-15_00C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20_00sec_-15_00C_LIGHT_0159_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4031 2461118.9031 10.65 16:53:30.12 -30:39:50.2
352.10494 8.29287 galactic Sco Second-epoch detections are separated by 0.3" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6027984061662492288 | 16:53:31.05 -30:40:01.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6027984061662492288,2461118.9031,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6027984061662492288 20260319.4031 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sco-02-Q2b1x1_045556_TTUQ2b1x1_22913_HE200OHy/fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sco-02-Q2b1x1_045556_TTUQ2b1x1_22913_HE200OHy/fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20.00sec_-15.00C_LIGHT_0159.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:53:30.12 -30:39:50.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20_00sec_-15_00C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20_00sec_-15_00C_LIGHT_0159_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4031 2461118.9031 10.69 16:44:06.03 -30:52:26.2
350.64824 9.72557 galactic Sco Second-epoch detections are separated by 0.4" 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 6030596226404116224 | 16:44:06.66 -30:52:28.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030596226404116224,2461118.9031,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6030596226404116224 20260319.4031 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sco-02-Q2b1x1_045556_TTUQ2b1x1_22913_HE200OHy/fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sco-02-Q2b1x1_045556_TTUQ2b1x1_22913_HE200OHy/fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20.00sec_-15.00C_LIGHT_0159.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:44:06.03 -30:52:26.2 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20_00sec_-15_00C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20_00sec_-15_00C_LIGHT_0159_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4031 2461118.9031 10.41 16:53:50.06 -28:50:14.9
353.60004 9.36927 galactic Oph Second-epoch detections are separated by 1.0" 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 6032784838677870336 | 16:53:50.19 -28:50:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.931+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032784838677870336,2461118.9031,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6032784838677870336 20260319.4031 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sco-02-Q2b1x1_045556_TTUQ2b1x1_22913_HE200OHy/fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Sco-02-Q2b1x1_045556_TTUQ2b1x1_22913_HE200OHy/fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20.00sec_-15.00C_LIGHT_0159.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:53:50.06 -28:50:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20_00sec_-15_00C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-40-42_20_00sec_-15_00C_LIGHT_0159_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-19_04-39-54_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4177 2461118.9177 14.24 20:44:49.57 +57:52:58.8
94.62949 9.29625 galactic Cep Second-epoch detections are separated by 4.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J311.1974+57.8837 | 20:44:49.57 +57:52:58.8 (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 J311.1974+57.8837,2461118.9177,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J311.1974+57.8837 20260319.4177 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20.00sec_-15.00C_LIGHT_0175.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:49.57 +57:52:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_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-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9177,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4177 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20.00sec_-15.00C_LIGHT_0175.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:27:17.08 +54:31:06.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_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-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4177 2461118.9177 13.63 21:58:11.96 +56:14:59.8
100.52635 1.10846 galactic Cep Second-epoch detections are separated by 1.4" 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 | Gaia DR3 2198166362350441600 | 21:58:16.94 +56:15:11.7 (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 2198166362350441600,2461118.9177,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2198166362350441600 20260319.4177 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20.00sec_-15.00C_LIGHT_0175.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:58:11.96 +56:14:59.8 ;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_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_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-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4177 2461118.9177 13.96 20:24:22.36 +48:53:35.5
85.48516 6.47395 galactic Cyg Second-epoch detections are separated by 3.1" 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 J306.0911+48.8966 | 20:24:21.49 +48:54:01.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J306.0911+48.8966,2461118.9177,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J306.0911+48.8966 20260319.4177 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20.00sec_-15.00C_LIGHT_0175.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:24:22.36 +48:53:35.5 ;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_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_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-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4177 2461118.9177 12.73 21:52:51.48 +52:41:44.7
97.71977 -1.20611 galactic Cyg Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J328.2089+52.7004 | 21:52:51.48 +52:41:44.7 (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 J328.2089+52.7004,2461118.9177,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J328.2089+52.7004 20260319.4177 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-01-28_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-02-Q2b1x1_2025-12-22_20-02-33_20.00sec_-14.90C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-02-Q2b1x1_050748_TTUQ2b1x1_16387_rEi3lMfU/fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20.00sec_-15.00C_LIGHT_0175.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:52:51.48 +52:41:44.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_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-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-01-59_20_00sec_-15_00C_LIGHT_0175_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-02-Q2b1x1_2025-12-22_20-01-28_20_00sec_-15_00C_LIGHT_0020_fits__*pix.png resample_wcs_fd_Cyg-02-Q2b1x1_2026-03-19_05-00-36_20_00sec_-14_90C_LIGHT_0174_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4285 2461118.9285 13.70 20:13:42.61 +37:13:53.3
74.71136 1.54370 galactic Cyg Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.4394+37.2355 | 20:13:42.61 +37:13:53.3 (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 J303.4394+37.2355,2461118.9285,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.4394+37.2355 20260319.4285 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20.00sec_-14.90C_LIGHT_0178.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20.00sec_-14.90C_LIGHT_0179.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:42.61 +37:13:53.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4285 2461118.9285 13.74 20:50:37.83 +37:09:09.1
79.00705 -4.42310 galactic Cyg Second-epoch detections are separated by 4.9" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J312.6645+37.1549 | 20:50:39.82 +37:08:58.0 (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 J312.6645+37.1549,2461118.9285,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.6645+37.1549 20260319.4285 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20.00sec_-14.90C_LIGHT_0178.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20.00sec_-14.90C_LIGHT_0179.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:50:37.83 +37:09:09.1 ;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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4285 2461118.9285 12.57 20:25:23.91 +40:46:53.6
78.92450 1.67476 galactic Cyg Second-epoch detections are separated by 5.8" 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 | ATO J306.3310+40.7906 | 20:25:22.51 +40:47:09.4 (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 J306.3310+40.7906,2461118.9285,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J306.3310+40.7906 20260319.4285 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20.00sec_-14.90C_LIGHT_0178.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20.00sec_-14.90C_LIGHT_0179.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:25:23.91 +40:46:53.6 ;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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4285 2461118.9285 13.85 21:09:37.96 +42:24:40.3
85.38512 -3.73307 galactic Cyg Second-epoch detections are separated by 3.1" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1969837551475152512 | 21:09:38.93 +42:25:16.5 (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 1969837551475152512,2461118.9285,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1969837551475152512 20260319.4285 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20.00sec_-14.90C_LIGHT_0178.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20.00sec_-14.90C_LIGHT_0179.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:09:37.96 +42:24:40.3 ;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-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4285 2461118.9285 13.93 20:09:55.73 +35:38:13.3
72.96053 1.30478 galactic Cyg Second-epoch detections are separated by 3.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J302.4812+35.6393 | 20:09:55.73 +35:38:13.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.4812+35.6393,2461118.9285,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J302.4812+35.6393 20260319.4285 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20.00sec_-14.90C_LIGHT_0178.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20.00sec_-14.90C_LIGHT_0179.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:09:55.73 +35:38:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4285 2461118.9285 13.94 20:15:00.90 +35:20:08.4
73.27861 0.27444 galactic Cyg Second-epoch detections are separated by 1.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.7654+35.3366 | 20:15:03.02 +35:19:46.6 (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 J303.7654+35.3366,2461118.9285,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.7654+35.3366 20260319.4285 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20.00sec_-14.90C_LIGHT_0178.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20.00sec_-14.90C_LIGHT_0179.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:15:00.90 +35:20:08.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4285 2461118.9285 14.05 20:22:23.78 +36:04:59.9
74.74039 -0.54240 galactic Cyg Second-epoch detections are separated by 2.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2057289270369759232 | 20:22:25.64 +36:05:25.4 (Gaia DR3) | BCEP (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2057289270369759232,2461118.9285,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2057289270369759232 20260319.4285 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20.00sec_-14.90C_LIGHT_0178.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20.00sec_-14.90C_LIGHT_0179.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:23.78 +36:04:59.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4285 2461118.9285 14.23 20:59:02.85 +34:28:25.4
78.03623 -7.44868 galactic Cyg Second-epoch detections are separated by 3.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J314.7598+34.4722 | 20:59:02.85 +34:28:25.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J314.7598+34.4722,2461118.9285,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J314.7598+34.4722 20260319.4285 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20.00sec_-14.90C_LIGHT_0178.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cyg-06-Q2b1x1_051846_TTUQ2b1x1_17860_xmOONLeQ/fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20.00sec_-14.90C_LIGHT_0179.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:59:02.85 +34:28:25.4 ;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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-17-32_20_00sec_-14_90C_LIGHT_0179_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Cyg-06-Q2b1x1_2026-03-19_05-16-20_20_00sec_-14_90C_LIGHT_0178_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4325* 01 23 05.59 +71 21 14.2 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9325,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4325 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-22_22-28-20_20.00sec_-15.00C_LIGHT_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-02-Q2b1x1_052416_TTUQ2b1x1_25158_jd3LgkLr/fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20.00sec_-15.00C_LIGHT_0182.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-02-Q2b1x1_052416_TTUQ2b1x1_25158_jd3LgkLr/fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20.00sec_-15.00C_LIGHT_0183.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:23:05.59 +71:21:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20_00sec_-15_00C_LIGHT_0183_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20_00sec_-15_00C_LIGHT_0183_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9325,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4325 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-22_22-28-20_20.00sec_-15.00C_LIGHT_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-02-Q2b1x1_052416_TTUQ2b1x1_25158_jd3LgkLr/fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20.00sec_-15.00C_LIGHT_0182.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-02-Q2b1x1_052416_TTUQ2b1x1_25158_jd3LgkLr/fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20.00sec_-15.00C_LIGHT_0183.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:44.49 +74:48:59.9 ;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_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20_00sec_-15_00C_LIGHT_0183_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20_00sec_-15_00C_LIGHT_0183_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9325,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4325 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-02-Q2b1x1_2025-12-22_22-28-20_20.00sec_-15.00C_LIGHT_0176.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-02-Q2b1x1_052416_TTUQ2b1x1_25158_jd3LgkLr/fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20.00sec_-15.00C_LIGHT_0182.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-02-Q2b1x1_052416_TTUQ2b1x1_25158_jd3LgkLr/fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20.00sec_-15.00C_LIGHT_0183.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:41:10.99 +80:37:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20_00sec_-15_00C_LIGHT_0183_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20_00sec_-15_00C_LIGHT_0182_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-23-10_20_00sec_-15_00C_LIGHT_0183_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-02-Q2b1x1_2025-12-22_22-28-20_20_00sec_-15_00C_LIGHT_0176_fits__*pix.png resample_wcs_fd_Cep-02-Q2b1x1_2026-03-19_05-21-59_20_00sec_-15_00C_LIGHT_0182_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4514* 23 05 21.28 +56 33 56.8 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9514,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4514 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:05:21.28 +56:33:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4514 2461118.9514 13.49 23:09:41.86 +56:36:27.3
109.23254 -3.53369 galactic Cas Second-epoch detections are separated by 4.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2009083205970997248 | 23:09:42.53 +56:36:29.9 (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!
TCP 2026 03 19.4514* 23 09 41.86 +56 36 27.3 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009083205970997248,2461118.9514,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009083205970997248 20260319.4514 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:09:41.86 +56:36:27.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4514 2461118.9514 13.55 22:33:23.20 +58:22:19.5
105.64706 0.21131 galactic Cep Second-epoch detections are separated by 1.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J338.3499+58.3710 | 22:33:26.80 +58:21:49.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J338.3499+58.3710,2461118.9514,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J338.3499+58.3710 20260319.4514 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:33:23.20 +58:22:19.5 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4514 2461118.9514 13.22 23:03:43.29 +56:32:26.1
108.44816 -3.27154 galactic Cas Second-epoch detections are separated by 2.4" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J345.9370+56.5427 | 23:03:43.29 +56:32:26.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4514* 23 03 43.29 +56 32 26.1 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J345.9370+56.5427,2461118.9514,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J345.9370+56.5427 20260319.4514 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:03:43.29 +56:32:26.1 ;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_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4514 2461118.9514 13.42 23:07:36.40 +56:43:09.1
109.01034 -3.31969 galactic Cas Second-epoch detections are separated by 2.2" 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 J346.8879+56.7201 | 23:07:35.32 +56:43:13.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4514* 23 07 36.40 +56 43 09.1 13.4 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
ATO J346.8879+56.7201,2461118.9514,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J346.8879+56.7201 20260319.4514 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:07:36.40 +56:43:09.1 ;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_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4514* 23 20 10.27 +61 08 47.5 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9514,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4514 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:20:10.27 +61:08:47.5 ;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_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4514* 23 21 08.52 +62 01 59.8 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9514,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4514 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:21:08.52 +62:01:59.8 ;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_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4514 2461118.9514 13.23 23:12:27.27 +57:05:51.1
109.76758 -3.22258 galactic Cas Second-epoch detections are separated by 0.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.1136+57.0997 | 23:12:27.27 +57:05:51.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4514* 23 12 27.27 +57 05 51.1 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.1136+57.0997,2461118.9514,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.1136+57.0997 20260319.4514 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 23:12:27.27 +57:05:51.1 ;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-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4514 2461118.9514 14.12 21:22:42.76 +60:24:05.2
99.76838 7.29307 galactic Cep Second-epoch detections are separated by 2.5" 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 | Gaia DR3 2191880454368469760 | 21:22:40.91 +60:23:23.0 (Gaia DR3) | DSCT/GDOR (local) | B (local) | Gaia3var=VARIABLE SpType: B8 1958TrRig...7...33A Cl Trumpler 37 1922
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2191880454368469760,2461118.9514,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2191880454368469760 20260319.4514 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-06-Q2b1x1_2025-12-22_21-00-50_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20.00sec_-15.00C_LIGHT_0194.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-06-Q2b1x1_055131_TTUQ2b1x1_30613_zblsub8a/fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20.00sec_-14.90C_LIGHT_0195.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:22:42.76 +60:24:05.2 ;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_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-50-30_20_00sec_-14_90C_LIGHT_0195_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-06-Q2b1x1_2025-12-22_21-00-50_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png resample_wcs_fd_Cep-06-Q2b1x1_2026-03-19_05-49-12_20_00sec_-15_00C_LIGHT_0194_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9582,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4582 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2025-12-26_19-03-23_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:25:39.77 +71:18:04.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9582,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4582 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2025-12-26_19-03-23_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:45:00.41 +73:25:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9582,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4582 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2025-12-26_19-03-23_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:21:06.11 +70:55:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4582 2461118.9582 13.79 21:36:36.92 +72:12:11.9
109.19494 14.75300 galactic Cep Second-epoch detections are separated by 2.0" 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 | Gaia DR3 2272942086554234752 | 21:36:35.03 +72:12:19.4 (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 2272942086554234752,2461118.9582,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2272942086554234752 20260319.4582 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2025-12-26_19-03-23_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:36:36.92 +72:12:11.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4582 2461118.9582 13.38 21:32:22.51 +72:08:37.9
108.91144 14.93669 galactic Cep Second-epoch detections are separated by 2.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2272985311105038848 | 21:32:21.03 +72:08:43.0 (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 2272985311105038848,2461118.9582,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2272985311105038848 20260319.4582 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2025-12-26_19-03-23_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:32:22.51 +72:08:37.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4582 2461118.9582 13.21 21:47:48.26 +73:09:55.3
110.50221 14.89794 galactic Cep Second-epoch detections are separated by 1.6" 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 | Large-amplitude variable Gaia DR2 2273110277474414976 | 21:47:46.50 +73:09:59.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2273110277474414976,2461118.9582,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2273110277474414976 20260319.4582 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2025-12-26_19-03-23_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:47:48.26 +73:09:55.3 ;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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9582,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4582 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2025-12-26_19-03-23_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:20:35.52 +81:50:12.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4582 2461118.9582 14.39 18:49:27.54 +72:57:55.9
103.91203 25.99103 galactic Dra 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 | Gaia DR3 2266149372438060672 | 18:49:24.08 +72:57:16.4 (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 2266149372438060672,2461118.9582,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2266149372438060672 20260319.4582 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2025-12-26_19-03-23_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-02-Q2b1x1_060116_TTUQ2b1x1_19293_mAItnubd/fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:49:27.54 +72:57:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_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_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_06-00-11_20_00sec_-14_90C_LIGHT_0202_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-02-Q2b1x1_2025-12-26_19-03-23_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Dra-02-Q2b1x1_2026-03-19_05-59-00_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4640 2461118.9640 10.54 15:40:41.64 +64:43:17.8
99.42109 43.89566 galactic Dra Second-epoch detections are separated by 0.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1641130922475867264 | 15:40:41.79 +64:43:17.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G 1956PMcCO..13a....B AG+64 739 J-Ks=0.488+/-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 1641130922475867264,2461118.9640,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1641130922475867264 20260319.4640 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q2b1x1_2025-12-23_06-12-29_20.00sec_-15.00C_LIGHT_0674.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-04-Q2b1x1_2025-12-23_06-13-06_20.00sec_-14.90C_LIGHT_0675.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-04-Q2b1x1_060946_TTUQ2b1x1_27105_t45oxU2F/fd_Dra-04-Q2b1x1_2026-03-19_06-07-26_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-04-Q2b1x1_060946_TTUQ2b1x1_27105_t45oxU2F/fd_Dra-04-Q2b1x1_2026-03-19_06-08-35_20.00sec_-14.90C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:40:41.64 +64:43:17.8 ;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_Dra-04-Q2b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q2b1x1_2026-03-19_06-08-35_20_00sec_-14_90C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-04-Q2b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q2b1x1_2026-03-19_06-07-26_20_00sec_-15_00C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q2b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q2b1x1_2026-03-19_06-08-35_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-04-Q2b1x1_2025-12-23_06-12-29_20_00sec_-15_00C_LIGHT_0674_fits__*pix.png resample_wcs_fd_Dra-04-Q2b1x1_2026-03-19_06-07-26_20_00sec_-15_00C_LIGHT_0207_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9679,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4679 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-04-Q2b1x1_061516_TTUQ2b1x1_12452_kn7dXDMw/fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-04-Q2b1x1_061516_TTUQ2b1x1_12452_kn7dXDMw/fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20.00sec_-15.00C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:42:32.41 +64:41:53.1 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20_00sec_-15_00C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20_00sec_-15_00C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20_00sec_-15_00C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20_00sec_-15_00C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4679 2461118.9679 12.94 22:30:59.81 +69:12:30.5
110.97950 9.66305 galactic Cep Second-epoch detections are separated by 2.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2226120723918718464 | 22:31:05.63 +69:11:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956PMcCO..13a....B AG+68 974
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2226120723918718464,2461118.9679,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2226120723918718464 20260319.4679 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-04-Q2b1x1_061516_TTUQ2b1x1_12452_kn7dXDMw/fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-04-Q2b1x1_061516_TTUQ2b1x1_12452_kn7dXDMw/fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20.00sec_-15.00C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:30:59.81 +69:12:30.5 ;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_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20_00sec_-15_00C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20_00sec_-15_00C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20_00sec_-15_00C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20_00sec_-15_00C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9679,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4679 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-22_20-27-30_20.00sec_-15.00C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-04-Q2b1x1_061516_TTUQ2b1x1_12452_kn7dXDMw/fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-04-Q2b1x1_061516_TTUQ2b1x1_12452_kn7dXDMw/fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20.00sec_-15.00C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:49:41.37 +65:12:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20_00sec_-15_00C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20_00sec_-15_00C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-14-12_20_00sec_-15_00C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-22_20-27-30_20_00sec_-15_00C_LIGHT_0048_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-19_06-13-00_20_00sec_-15_00C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 9.31 20:23:19.53 +65:26:47.9
99.51667 15.68901 galactic Dra Second-epoch detections are separated by 0.3" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2244745076503100032 | 20:23:20.66 +65:26:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2244745076503100032,2461118.9660,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2244745076503100032 20260319.4660 9.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:23:19.53 +65:26:47.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 10.59 20:09:53.49 +65:31:39.7
98.85872 16.93360 galactic Dra Second-epoch detections are separated by 0.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2247903148775052928 | 20:09:52.45 +65:31:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2247903148775052928,2461118.9660,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2247903148775052928 20260319.4660 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:09:53.49 +65:31:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 11.61 20:04:26.94 +65:37:40.8
98.67293 17.47676 galactic Dra Second-epoch detections are separated by 0.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx2585995 | 20:04:26.94 +65:37:41.0 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.704+/-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
DocumentRef: VOTx2585995,2461118.9660,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2585995 20260319.4660 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 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:04:26.94 +65:37:40.8 ;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-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 11.57 20:12:50.40 +68:07:25.4
101.39037 17.92828 galactic Dra Second-epoch detections are separated by 0.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J201246.95+680705.1 | 20:12:46.99 +68:07:05.1 (Gaia DR3) | L (local) | d (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 J201246.95+680705.1,2461118.9660,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201246.95+680705.1 20260319.4660 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 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:50.40 +68:07:25.4 ;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_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 11.60 20:22:43.70 +64:48:00.3
98.91133 15.40290 galactic Dra Second-epoch detections are separated by 0.5" 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 2244654813466764544 | 20:22:44.75 +64:47:55.3 (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 2244654813466764544,2461118.9660,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2244654813466764544 20260319.4660 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:43.70 +64:48:00.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 12.60 19:58:15.79 +65:02:30.2
97.81722 17.78509 galactic Dra Second-epoch detections are separated by 1.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2247535151679497472 | 19:58:16.31 +65:02:25.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3.5 2013AJ....145..102L PM J19582+6502
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2247535151679497472,2461118.9660,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2247535151679497472 20260319.4660 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:15.79 +65:02:30.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9660,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4660 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:19.50 +65:52:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9660,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4660 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:21:12.45 +65:34:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 12.05 20:19:19.42 +66:06:00.5
99.87748 16.37844 galactic Dra Second-epoch detections are separated by 0.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2246475570364047616 | 20:19:19.24 +66:06:01.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.222+/-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 2246475570364047616,2461118.9660,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2246475570364047616 20260319.4660 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 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-58-25_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:19.42 +66:06:00.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 12.54 19:58:13.26 +65:16:24.1
98.03306 17.89215 galactic Dra Second-epoch detections are separated by 0.1" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2247542264144413824 | 19:58:13.29 +65:16:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-0.025 (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 2247542264144413824,2461118.9660,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2247542264144413824 20260319.4660 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 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-58-25_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:58:13.26 +65:16:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 12.03 20:12:52.21 +65:03:13.3
98.58507 16.43076 galactic Dra Second-epoch detections are separated by 0.3" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2244870695706159488 | 20:12:52.17 +65:03:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.674+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2244870695706159488,2461118.9660,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2244870695706159488 20260319.4660 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 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-58-25_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:12:52.21 +65:03:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 11.98 20:22:59.65 +66:00:31.0
99.99591 16.01218 galactic Dra Second-epoch detections are separated by 0.4" 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 2246461654670052992 | 20:22:59.12 +66:00:33.9 (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 2246461654670052992,2461118.9660,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2246461654670052992 20260319.4660 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-58-25_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:22:59.65 +66:00:31.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4660 2461118.9660 10.81 20:13:13.51 +65:40:57.9
99.17526 16.70840 galactic Dra Second-epoch detections are separated by 0.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2244994459483177472 | 20:13:13.69 +65:40:57.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.036+/-9.995 (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 2244994459483177472,2461118.9660,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2244994459483177472 20260319.4660 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-57-47_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-01-09_02-58-25_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-05-Q2b1x1_061231_TTUQ2b1x1_14537_mTI0tx7t/fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:13:13.51 +65:40:57.9 ;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_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-11-23_20_00sec_-14_90C_LIGHT_0210_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-01-09_02-57-47_20_00sec_-14_90C_LIGHT_0032_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9844,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4844 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/UMa-05-Q2b1x1_2025-12-23_04-37-20_20.00sec_-15.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-05-Q2b1x1_063901_TTUQ2b1x1_1097_HlQA1Wjp/fd_UMa-05-Q2b1x1_2026-03-19_06-36-48_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_UMa-05-Q2b1x1_063901_TTUQ2b1x1_1097_HlQA1Wjp/fd_UMa-05-Q2b1x1_2026-03-19_06-38-00_20.00sec_-14.90C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:33:14.12 +65:12:02.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_UMa-05-Q2b1x1_2025-12-23_04-37-20_20_00sec_-15_00C_LIGHT_0566_fits__*pix.png resample_wcs_fd_UMa-05-Q2b1x1_2026-03-19_06-38-00_20_00sec_-14_90C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_UMa-05-Q2b1x1_2025-12-23_04-37-20_20_00sec_-15_00C_LIGHT_0566_fits__*pix.png resample_wcs_fd_UMa-05-Q2b1x1_2026-03-19_06-36-48_20_00sec_-15_00C_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_UMa-05-Q2b1x1_2025-12-23_04-37-20_20_00sec_-15_00C_LIGHT_0566_fits__*pix.png resample_wcs_fd_UMa-05-Q2b1x1_2026-03-19_06-38-00_20_00sec_-14_90C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_UMa-05-Q2b1x1_2025-12-23_04-37-20_20_00sec_-15_00C_LIGHT_0566_fits__*pix.png resample_wcs_fd_UMa-05-Q2b1x1_2026-03-19_06-36-48_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4904 2461118.9904 14.38 18:05:14.05 +58:05:23.5
86.71766 28.76868 galactic Dra Second-epoch detections are separated by 1.0" and 0.9 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 | 18:05:14.05 +58:05:23.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9904,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4904 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-07-Q2b1x1_2025-12-23_06-37-17_20.00sec_-15.00C_LIGHT_0702.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-07-Q2b1x1_064746_TTUQ2b1x1_4884_9ds86Ic6/fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-07-Q2b1x1_064746_TTUQ2b1x1_4884_9ds86Ic6/fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20.00sec_-14.90C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:05:14.05 +58:05:23.5 ;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_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20_00sec_-14_90C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20_00sec_-15_00C_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_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20_00sec_-15_00C_LIGHT_0227_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4904 2461118.9904 13.90 17:42:38.29 +62:37:18.6
91.83420 31.73112 galactic Dra Second-epoch detections are separated by 5.3" 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 | Gaia DR3 1439540928721399808 | 17:42:41.16 +62:37:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1439540928721399808,2461118.9904,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1439540928721399808 20260319.4904 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-07-Q2b1x1_2025-12-23_06-37-17_20.00sec_-15.00C_LIGHT_0702.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-07-Q2b1x1_064746_TTUQ2b1x1_4884_9ds86Ic6/fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-07-Q2b1x1_064746_TTUQ2b1x1_4884_9ds86Ic6/fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20.00sec_-14.90C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:42:38.29 +62:37:18.6 ;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_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20_00sec_-14_90C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20_00sec_-15_00C_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_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20_00sec_-15_00C_LIGHT_0227_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.9904,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.4904 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-07-Q2b1x1_2025-12-23_06-37-17_20.00sec_-15.00C_LIGHT_0702.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-07-Q2b1x1_064746_TTUQ2b1x1_4884_9ds86Ic6/fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-07-Q2b1x1_064746_TTUQ2b1x1_4884_9ds86Ic6/fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20.00sec_-14.90C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:41:12.78 +60:27:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20_00sec_-14_90C_LIGHT_0228_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20_00sec_-15_00C_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_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-46-33_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-07-Q2b1x1_2025-12-23_06-37-17_20_00sec_-15_00C_LIGHT_0702_fits__*pix.png resample_wcs_fd_Dra-07-Q2b1x1_2026-03-19_06-45-22_20_00sec_-15_00C_LIGHT_0227_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4923 2461118.9923 9.60 19:42:19.98 +60:21:52.7
92.56560 17.42208 galactic Dra Second-epoch detections are separated by 0.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 2239073585069039488,2461118.9923,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2239073585069039488 20260319.4923 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 /data_ssd/NMW-TexasTech/reference_imgs/Dra-08-Q2b1x1_2026-01-09_03-33-26_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-08-Q2b1x1_065031_TTUQ2b1x1_10711_QAtja2bd/fd_Dra-08-Q2b1x1_2026-03-19_06-48-09_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Dra-08-Q2b1x1_065031_TTUQ2b1x1_10711_QAtja2bd/fd_Dra-08-Q2b1x1_2026-03-19_06-49-22_20.00sec_-14.90C_LIGHT_0230.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:19.98 +60:21:52.7 ;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_Dra-08-Q2b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q2b1x1_2026-03-19_06-49-22_20_00sec_-14_90C_LIGHT_0230_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-08-Q2b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q2b1x1_2026-03-19_06-48-09_20_00sec_-15_00C_LIGHT_0229_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-08-Q2b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q2b1x1_2026-03-19_06-49-22_20_00sec_-14_90C_LIGHT_0230_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-08-Q2b1x1_2026-01-09_03-33-26_20_00sec_-15_00C_LIGHT_0062_fits__*pix.png resample_wcs_fd_Dra-08-Q2b1x1_2026-03-19_06-48-09_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.5002 2461119.0002 13.43 21:27:51.03 +57:33:33.2
98.23991 4.80196 galactic Cep Second-epoch detections are separated by 2.8" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J321.9590+57.5596 | 21:27:50.17 +57:33:34.8 (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 J321.9590+57.5596,2461119.0002,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J321.9590+57.5596 20260319.5002 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-05-Q2b1x1_070116_TTUQ2b1x1_13162_ZodAlpwK/fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-05-Q2b1x1_070116_TTUQ2b1x1_13162_ZodAlpwK/fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:27:51.03 +57:33:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20_00sec_-14_90C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20_00sec_-14_90C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.5002 2461119.0002 12.86 21:26:32.11 +56:44:41.4
97.54380 4.33985 galactic Cep Second-epoch detections are separated by 3.2" and 0.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2178680164443939584 | 21:26:31.30 +56:44:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2178680164443939584,2461119.0002,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2178680164443939584 20260319.5002 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-05-Q2b1x1_070116_TTUQ2b1x1_13162_ZodAlpwK/fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-05-Q2b1x1_070116_TTUQ2b1x1_13162_ZodAlpwK/fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:26:32.11 +56:44:41.4 ;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-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20_00sec_-14_90C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20_00sec_-14_90C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.0002,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.5002 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-05-Q2b1x1_070116_TTUQ2b1x1_13162_ZodAlpwK/fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-05-Q2b1x1_070116_TTUQ2b1x1_13162_ZodAlpwK/fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:17:14.33 +66:08:37.4 ;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_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20_00sec_-14_90C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20_00sec_-14_90C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.0002,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.5002 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q2b1x1_2025-12-22_19-47-11_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-05-Q2b1x1_070116_TTUQ2b1x1_13162_ZodAlpwK/fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cep-05-Q2b1x1_070116_TTUQ2b1x1_13162_ZodAlpwK/fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20.00sec_-14.90C_LIGHT_0234.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:59:26.95 +58:02:54.4 ;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_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20_00sec_-14_90C_LIGHT_0234_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_07-00-31_20_00sec_-14_90C_LIGHT_0234_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-05-Q2b1x1_2025-12-22_19-47-11_20_00sec_-15_00C_LIGHT_0004_fits__*pix.png resample_wcs_fd_Cep-05-Q2b1x1_2026-03-19_06-59-47_20_00sec_-15_00C_LIGHT_0233_fits__*pix.png animation_v2.gif