Mean magnitude and position on the discovery images:
2026 02 27.3839 2461098.8839 11.87 17:39:31.91 -14:39:02.8
11.49895 8.65087 galactic Ser Second-epoch detections are separated by 3.1" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4149248955591882112 | 17:39:32.33 -14:39:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3839* 17 39 31.91 -14 39 02.8 11.9 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4149248955591882112,2461098.8839,11.87,0.05,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 4149248955591882112 20260227.3839 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/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:39:31.91 -14:39:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3839 2461098.8839 12.55 17:38:33.40 -05:02:34.5
19.82796 13.71633 galactic Oph Second-epoch detections are separated by 0.6" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J264.6435-05.0420 | 17:38:33.75 -05:02:28.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J264.6435-05.0420,2461098.8839,12.55,0.05,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 J264.6435-05.0420 20260227.3839 12.55CV 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/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:38:33.40 -05:02:34.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 27.3839* 17 29 41.05 -14 33 59.9 13.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.8839,12.96,0.05,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
target 20260227.3839 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/Oph-05-Q2b1x1_2026-01-18_05-49-04_20.00sec_-14.90C_LIGHT_0549.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20.00sec_-15.00C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Oph-05-Q2b1x1_063645_TTUQ2b1x1_12866_Pn4C7fpX/fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20.00sec_-15.00C_LIGHT_0167.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:29:41.05 -14:33:59.9 ;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_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-13-00_20_00sec_-15_00C_LIGHT_0167_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-05-Q2b1x1_2026-01-18_05-49-04_20_00sec_-14_90C_LIGHT_0549_fits__*pix.png resample_wcs_fd_Oph-05-Q2b1x1_2026-02-27_03-12-16_20_00sec_-15_00C_LIGHT_0166_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5162 2461099.0162 10.37 17:25:17.90 -22:03:13.6
3.35503 7.56043 galactic Oph 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 | ATO J261.3328-22.0509 | 17:25:18.33 -22:03:15.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J261.3328-22.0509,2461099.0162,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J261.3328-22.0509 20260227.5162 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-01-18_06-03-32_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-07-Q2b1x1_172749_TTUQ2b1x1_29888_rDLpoPOR/fd_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-07-Q2b1x1_172749_TTUQ2b1x1_29888_rDLpoPOR/fd_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:25:17.90 -22:03:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-02-27_06-23-33_20_00sec_-15_00C_LIGHT_0322_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_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_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_2026-02-27_06-23-33_20_00sec_-15_00C_LIGHT_0322_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_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5162 2461099.0162 11.19 17:23:49.09 -20:42:43.8
4.29518 8.58621 galactic Oph Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 | 17:23:48.60 -20:42:43.2 (Gaia DR3) | 4121134060981623552 (VSX @ VizieR) | RRC (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE SpType: A3 1939AnBos...5E...1W CPD-20 6556 J-Ks=0.869+/-0.036 (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 DR3,2461099.0162,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 20260227.5162 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-01-18_06-03-32_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-07-Q2b1x1_172749_TTUQ2b1x1_29888_rDLpoPOR/fd_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-07-Q2b1x1_172749_TTUQ2b1x1_29888_rDLpoPOR/fd_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:23:49.09 -20:42:43.8 ;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_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-02-27_06-23-33_20_00sec_-15_00C_LIGHT_0322_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_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_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_2026-02-27_06-23-33_20_00sec_-15_00C_LIGHT_0322_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_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5162 2461099.0162 11.27 17:20:53.53 -22:59:15.0
2.00153 7.88956 galactic Oph Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4114615748082052864 | 17:20:53.92 -22:59:17.6 (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 4114615748082052864,2461099.0162,11.27,0.05,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 4114615748082052864 20260227.5162 11.27CV 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/Oph-07-Q2b1x1_2026-01-18_06-03-32_20.00sec_-15.00C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-07-Q2b1x1_172749_TTUQ2b1x1_29888_rDLpoPOR/fd_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-07-Q2b1x1_172749_TTUQ2b1x1_29888_rDLpoPOR/fd_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:20:53.53 -22:59:15.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-02-27_06-23-33_20_00sec_-15_00C_LIGHT_0322_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_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_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_2026-02-27_06-23-33_20_00sec_-15_00C_LIGHT_0322_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_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5162 2461099.0162 11.42 17:21:09.92 -19:35:16.5
4.89786 9.72531 galactic Oph Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J260.2975-19.5823 | 17:21:09.92 -19:35:16.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3/4 CN4 1985PASP...97..465H NGC 6342 J-Ks=0.863+/-0.136 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J260.2975-19.5823,2461099.0162,11.42,0.05,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 J260.2975-19.5823 20260227.5162 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-10_CI_Oph-07-Q2b1x1_172749_TTUQ2b1x1_29888_rDLpoPOR/fd_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-07-Q2b1x1_172749_TTUQ2b1x1_29888_rDLpoPOR/fd_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:21:09.92 -19:35:16.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-07-Q2b1x1_2026-01-18_06-03-32_20_00sec_-15_00C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-02-27_06-23-33_20_00sec_-15_00C_LIGHT_0322_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_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_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_2026-02-27_06-23-33_20_00sec_-15_00C_LIGHT_0322_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_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5149 2461099.0149 8.43 18:28:02.78 -14:39:36.1
17.25032 -1.58585 galactic Sct Second-epoch detections are separated by 1.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J277.0207-14.6617 | 18:28:03.21 -14:39:38.4 (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 J277.0207-14.6617,2461099.0149,8.43,0.05,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 J277.0207-14.6617 20260227.5149 8.43CV 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/Oph-06-Q2b1x1_2026-01-18_06-39-24_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:28:02.78 -14:39:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5149 2461099.0149 9.36 18:26:27.11 -13:11:28.1
18.37081 -0.56003 galactic Sct Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4152516459291000960 | 18:26:26.97 -13:11:34.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1935MeUpp..61....1S BD-13 4978
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4152516459291000960,2461099.0149,9.36,0.05,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 4152516459291000960 20260227.5149 9.36CV 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/Oph-06-Q2b1x1_2026-01-18_06-39-24_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:26:27.11 -13:11:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5149 2461099.0149 9.71 17:30:00.16 -04:48:13.2
18.95064 15.68527 galactic Oph Second-epoch detections are separated by 0.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J262.4935-04.8086 | 17:29:59.84 -04:48:09.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0 1945AJ.....51..187G BD-04 4289
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J262.4935-04.8086,2461099.0149,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J262.4935-04.8086 20260227.5149 9.71CV 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/Oph-06-Q2b1x1_2026-01-18_06-39-24_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:30:00.16 -04:48:13.2 ;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_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5149 2461099.0149 9.94 18:28:55.86 -14:33:54.4
17.43376 -1.73142 galactic Sct Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4104134683504996736 | 18:28:56.43 -14:33:57.1 (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 4104134683504996736,2461099.0149,9.94,0.05,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 4104134683504996736 20260227.5149 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:28:55.86 -14:33:54.4 ;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_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5149 2461099.0149 10.17 18:27:22.26 -15:01:08.2
16.85652 -1.60805 galactic Sct Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J276.8410-15.0121 | 18:27:22.67 -15:01:10.8 (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 J276.8410-15.0121,2461099.0149,10.17,0.05,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
ATO J276.8410-15.0121 20260227.5149 10.17CV 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/Oph-06-Q2b1x1_2026-01-18_06-39-24_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:27:22.26 -15:01:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5149 2461099.0149 10.47 18:30:24.35 -14:47:00.4
17.40525 -2.14865 galactic Sct Second-epoch detections are separated by 0.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J277.6024-14.7764 | 18:30:24.82 -14:47:04.8 (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 J277.6024-14.7764,2461099.0149,10.47,0.05,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 J277.6024-14.7764 20260227.5149 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-01-18_06-39-24_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:30:24.35 -14:47:00.4 ;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_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5149 2461099.0149 11.01 18:30:29.83 -09:41:51.9
21.92477 0.18535 galactic Sct Second-epoch detections are separated by 2.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4155870111503491712 | 18:30:30.27 -09:41:49.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4155870111503491712,2461099.0149,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4155870111503491712 20260227.5149 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:30:29.83 -09:41:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.5149 2461099.0149 10.19 18:16:33.51 -13:53:43.7
16.61786 1.23032 galactic Ser Second-epoch detections are separated by 0.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4146630193732750592 | 18:16:33.54 -13:53:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.955+/-0.036 (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 02 27.5149* 18 16 33.51 -13 53 43.7 10.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146630193732750592,2461099.0149,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146630193732750592 20260227.5149 10.19CV 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/Oph-06-Q2b1x1_2026-01-18_06-39-24_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-06-Q2b1x1_2026-01-18_06-40-09_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-20-53_20.00sec_-14.90C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-10_CI_Oph-06-Q2b1x1_041913_TTUQ2b1x1_17835_QqRsStxr/fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20.00sec_-15.00C_LIGHT_0320.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:16:33.51 -13:53:43.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-06-Q2b1x1_2026-01-18_06-39-24_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Oph-06-Q2b1x1_2026-02-27_06-21-43_20_00sec_-15_00C_LIGHT_0320_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_2026-02-27_06-20-53_20_00sec_-14_90C_LIGHT_0319_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3152 2461098.8152 9.44 14:57:09.96 -27:35:35.0
334.33557 27.50403 galactic Hya Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6225267783717101056 | 14:57:10.01 -27:35:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.714+/-0.029 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6225267783717101056,2461098.8152,9.44,0.05,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
Gaia DR3 6225267783717101056 20260227.3152 9.44CV 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/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_2026-02-28_CI_Hya-14-Q2b1x1_044244_TTUQ2b1x1_26402_U1o9F2mm/fd_Hya-14-Q2b1x1_2026-02-27_01-33-07_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-28_CI_Hya-14-Q2b1x1_044244_TTUQ2b1x1_26402_U1o9F2mm/fd_Hya-14-Q2b1x1_2026-02-27_01-34-21_20.00sec_-14.90C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:57:09.96 -27:35:35.0 ;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_Hya-14-Q2b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-02-27_01-34-21_20_00sec_-14_90C_LIGHT_0058_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_2026-02-27_01-33-07_20_00sec_-15_00C_LIGHT_0057_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_2026-02-27_01-34-21_20_00sec_-14_90C_LIGHT_0058_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_2026-02-27_01-33-07_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3152 2461098.8152 11.85 14:57:33.59 -27:19:52.9
334.57435 27.68104 galactic Hya Second-epoch detections are separated by 0.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6225298604402846336 | 14:57:33.65 -27:19:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6225298604402846336,2461098.8152,11.85,0.05,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 6225298604402846336 20260227.3152 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-02-28_CI_Hya-14-Q2b1x1_044244_TTUQ2b1x1_26402_U1o9F2mm/fd_Hya-14-Q2b1x1_2026-02-27_01-33-07_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-28_CI_Hya-14-Q2b1x1_044244_TTUQ2b1x1_26402_U1o9F2mm/fd_Hya-14-Q2b1x1_2026-02-27_01-34-21_20.00sec_-14.90C_LIGHT_0058.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:57:33.59 -27:19:52.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-14-Q2b1x1_2026-01-09_04-32-00_20_00sec_-14_90C_LIGHT_0095_fits__*pix.png resample_wcs_fd_Hya-14-Q2b1x1_2026-02-27_01-34-21_20_00sec_-14_90C_LIGHT_0058_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_2026-02-27_01-33-07_20_00sec_-15_00C_LIGHT_0057_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_2026-02-27_01-34-21_20_00sec_-14_90C_LIGHT_0058_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_2026-02-27_01-33-07_20_00sec_-15_00C_LIGHT_0057_fits__*pix.png animation_v2.gif